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Class D Audio Amplifier The design of a live audio Class D audio amplifier with greater than 90% efficiency and less than 1% distortion. A Major Qualifying Project Submitted to the Faculty of the WORCESTER POLYTECHNIC INSTITUTE in partial fulfillment of the requirements for the Degree of Bachelor of Science in Electrical Engineering by Briana Morey Ravi Vasudevan Ian Woloschin May 2008 APPROVED: Professor John McNeill, Advisor Professor Andrew Klein, Advisor

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Page 1: Class D Audio Amplifier - m.wpi.edu

Class D Audio Amplifier

The design of a live audio Class D audio amplifier with greater than 90%efficiency and less than 1% distortion.

A Major Qualifying Project

Submitted to the Faculty

of the

WORCESTER POLYTECHNIC INSTITUTE

in partial fulfillment of the requirements for the

Degree of Bachelor of Science

in

Electrical Engineering

by

Briana Morey

Ravi Vasudevan

Ian Woloschin

May 2008

APPROVED:

Professor John McNeill, Advisor Professor Andrew Klein, Advisor

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Abstract

The purpose of this project was to design and produce a 90% efficient, 80W Class D audioamplifier, with less than 1% Total Harmonic Distortion (THD) for the NECAMSID Lab.The amplifier consisted of a second order, three-level ∆Σ modulator, an H-bridge powerstage, and a second order, passive Butterworth filter. Testing confirmed that the efficiency,THD, and power specifications were met in the final revision of the design.

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ACKNOWLEDGEMENTS

We would like to thank Professor McNeill and Professor Klein for advising this project. Wewould also like to thank the NECAMSID lab for sponsoring this project.

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Contents

1 Introduction 11.1 Project Objectives . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21.2 Report Organization . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2

2 Background 32.1 Class D Amplification . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3

2.1.1 Operation of Class D Audio Amplifiers . . . . . . . . . . . . . . . . . 42.1.2 Advantages and Disadvantages of Class D . . . . . . . . . . . . . . . 62.1.3 Applying Class D to Audio Design . . . . . . . . . . . . . . . . . . . 7

2.2 The Modulation Stage . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82.2.1 Pulse Width Modulation (PWM) . . . . . . . . . . . . . . . . . . . . 92.2.2 Delta Sigma Modulation (∆Σ) . . . . . . . . . . . . . . . . . . . . . . 10

2.3 The Power Stage . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 122.3.1 Half-Bridge Amplifiers . . . . . . . . . . . . . . . . . . . . . . . . . . 122.3.2 H-Bridge Amplifiers . . . . . . . . . . . . . . . . . . . . . . . . . . . 132.3.3 A Critical Evaluation of Half- and H-Bridge Amplifiers . . . . . . . . 142.3.4 MOSFET Drivers . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15

2.4 Noise and the Filtering Stage . . . . . . . . . . . . . . . . . . . . . . . . . . 152.4.1 Types of Noise . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 162.4.2 Passive Filters vs. Active Filters . . . . . . . . . . . . . . . . . . . . . 192.4.3 Single Ended Filters vs. Balanced Filters . . . . . . . . . . . . . . . . 20

3 Preliminary Design 223.1 The Modulation Stage . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 22

3.1.1 The First Order Delta Sigma Modulator Design . . . . . . . . . . . . 233.2 The Power Stage . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 26

3.2.1 Amplifier Configuration . . . . . . . . . . . . . . . . . . . . . . . . . 263.2.2 MOSFET Selection . . . . . . . . . . . . . . . . . . . . . . . . . . . . 263.2.3 MOSFET Drivers . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 30

3.3 Filter . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 313.3.1 Filter Components . . . . . . . . . . . . . . . . . . . . . . . . . . . . 32

3.4 System Implementation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 343.4.1 First Order Modulator . . . . . . . . . . . . . . . . . . . . . . . . . . 343.4.2 PCB Layout for Power Stage and Filter . . . . . . . . . . . . . . . . . 353.4.3 Full System Assembly . . . . . . . . . . . . . . . . . . . . . . . . . . 36

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4 Preliminary Results 384.1 Functionality Testing . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 38

4.1.1 Modulator Functionality . . . . . . . . . . . . . . . . . . . . . . . . . 394.1.2 Power Stage Functionality . . . . . . . . . . . . . . . . . . . . . . . . 404.1.3 Filter Functionality . . . . . . . . . . . . . . . . . . . . . . . . . . . . 414.1.4 System Functionality . . . . . . . . . . . . . . . . . . . . . . . . . . . 44

4.2 Efficiency Testing . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 454.3 Frequency Response Testing . . . . . . . . . . . . . . . . . . . . . . . . . . . 464.4 Problems with the Preliminary Design and Tests . . . . . . . . . . . . . . . . 49

5 Final Design 515.1 The Second Order Modulator . . . . . . . . . . . . . . . . . . . . . . . . . . 51

5.1.1 System Model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 525.1.2 Physical Realization . . . . . . . . . . . . . . . . . . . . . . . . . . . 525.1.3 Modulation Frequency . . . . . . . . . . . . . . . . . . . . . . . . . . 57

5.2 The Power Stage . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 585.3 Filter . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 58

5.3.1 Capacitor Microphonics . . . . . . . . . . . . . . . . . . . . . . . . . 595.3.2 Cut-Off Frequency . . . . . . . . . . . . . . . . . . . . . . . . . . . . 595.3.3 New Inductors . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 605.3.4 Filter Configuration . . . . . . . . . . . . . . . . . . . . . . . . . . . . 60

5.4 Final PCB Layout . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 61

6 Final Results 646.1 Functionality Test Results . . . . . . . . . . . . . . . . . . . . . . . . . . . . 64

6.1.1 Modulator . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 656.1.2 Power Stage . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 656.1.3 Filter . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 66

6.2 Efficiency Results . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 676.3 Sound Quality Results . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 68

6.3.1 Loopback Test . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 706.3.2 Total Harmonic Distortion . . . . . . . . . . . . . . . . . . . . . . . . 726.3.3 Signal To Noise Ratio . . . . . . . . . . . . . . . . . . . . . . . . . . 736.3.4 Frequency Response . . . . . . . . . . . . . . . . . . . . . . . . . . . 746.3.5 Listening Test . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 75

7 Conclusion 77

8 Future Work & Recommendations 808.1 High Efficiency Power Supply . . . . . . . . . . . . . . . . . . . . . . . . . . 808.2 PCB Modulator with Full System Feedback . . . . . . . . . . . . . . . . . . 818.3 Digital Input . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 818.4 Multichannel Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82

A First Order ∆Σ Modulation: Matlab Simulation Code 86

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B Matlab Script to Find ‘a’ Coefficients 89

C First Order ∆Σ Modulation: Matlab Simulation Code 91

D MOSFET Equation Derivations 94

E MOSFET Losses: Matlab Simulation Code 100

F MOSFET Data Sheet 106

G Preliminary Schematic 116

H Final Schematics 117

I Final Matlab Test Code 120I.1 Efficiency . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 120I.2 THD . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 123I.3 SNR . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 125

J Preliminary Efficiency Test Results 127

K Final Efficiency Test Results 131

L Final Sound Quality Test Results 140L.1 Loopback Results . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 141L.2 Signal Quality Results with 1MHz Modulation Frequency . . . . . . . . . . . 142L.3 Signal Quality Results with 2MHz Modulation Frequency . . . . . . . . . . . 143L.4 Signal Quality Results with 5MHz Modulation Frequency . . . . . . . . . . . 145L.5 Signal Quality Results with 10MHz Modulation Frequency . . . . . . . . . . 146

M Digital Audio 148

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List of Figures

2.1 A Class A audio amplifier. . . . . . . . . . . . . . . . . . . . . . . . . . . . . 42.2 Block Diagram of a Class D Amplifier . . . . . . . . . . . . . . . . . . . . . . 62.3 A system model of a first order ∆Σ Modulator. . . . . . . . . . . . . . . . . 102.4 A system model of a first order ∆Σ Modulator after the quantizer is replaced

with additive quantization noise for modelling and simulation. . . . . . . . . 102.5 An approximate representation of the signal (red) and noise (blue) transfer

functions of a simple delta sigma modulator. . . . . . . . . . . . . . . . . . . 112.6 A Half-Bridge Amplifier . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 132.7 An H-Bridge Amplifier . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 132.8 A 2kHz signal modulated at 10MHz with delta sigma modulation. . . . . . . 162.9 A basic active low pass filter. . . . . . . . . . . . . . . . . . . . . . . . . . . 192.10 A basic passive low pass filter. . . . . . . . . . . . . . . . . . . . . . . . . . . 192.11 Single Ended and Balanced Filter [McD01] . . . . . . . . . . . . . . . . . . . 21

3.1 The schematic used to simulate a first order delta sigma modulator. . . . . . 233.2 The results of the first order delta sigma simulation, conducted with a 2kHz

sine wave and a 1MHz modulation frequency. . . . . . . . . . . . . . . . . . 253.3 A MOSFET timing diagram. . . . . . . . . . . . . . . . . . . . . . . . . . . . 283.4 The curves for each simulated MOSFET. . . . . . . . . . . . . . . . . . . . . 303.5 Half circuit model of the second order Butterworth filter.[TI:99] . . . . . . . 323.6 The bread-board containing the modulator shown in the schematic in Figure 3.1. 343.7 The PCB of the Power Stage without Components . . . . . . . . . . . . . . 353.8 The PCB of the Power Stage with soldered components Components . . . . 363.9 The Resistor Used for Testing . . . . . . . . . . . . . . . . . . . . . . . . . . 363.10 The PCB of the Power Stage without Components . . . . . . . . . . . . . . 37

4.1 The Matlab simulation of the first order modulator. . . . . . . . . . . . . . 394.2 The output of the first order delta sigma modulator, with a 1MHz modulation

frequency and a 10kHz sine wave. . . . . . . . . . . . . . . . . . . . . . . . . 404.3 The Power Stage Output . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 414.4 The configuration of the test resistor and the oscilloscope probes. . . . . . . 424.5 The power stage and filter with a 1kHz square wave input . . . . . . . . . . 434.6 The power stage and filter with a 10kHz square wave input. . . . . . . . . . 434.7 The full system with a 1kHz sine wave input. . . . . . . . . . . . . . . . . . . 444.8 The full system with a 10kHz sine wave input. . . . . . . . . . . . . . . . . . 454.9 Efficiency Plot at 11VRMS at the Output . . . . . . . . . . . . . . . . . . . . 46

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4.10 Efficiency Plot at 25VRMS at the Output . . . . . . . . . . . . . . . . . . . . 474.11 Efficiency Plot at 50Hz . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 474.12 Efficiency Plot at 1200Hz . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 484.13 Efficiency Plot at all Frequencies and Output Voltages . . . . . . . . . . . . 484.14 Frequency Response Plots . . . . . . . . . . . . . . . . . . . . . . . . . . . . 49

5.1 The discrete model of a second order delta sigma modulator [ST05]. . . . . . 535.2 The results of the system model simulation after adjusting the coefficients. . 535.3 The intermediate stage between the Matlab simulation of the system model

and the final system. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 545.4 The output of the intermediate stage between the Matlab simulation of the

system model and the final system. . . . . . . . . . . . . . . . . . . . . . . . 555.5 The Fast-Fourier Transform (FFT) of the intermediate stage output. . . . . 555.6 The final spice simulation of the second order delta sigma modulator. . . . . 565.7 The output of the second order three-level modulator on a bread-board . . . 575.8 Addition of Electrolytic Bypass Capacitor at Rails . . . . . . . . . . . . . . . 585.9 Addition of Tantalum Bypass Capacitor at MOSFET . . . . . . . . . . . . . 585.10 Preliminary Filter Design . . . . . . . . . . . . . . . . . . . . . . . . . . . . 605.11 Final Filter Design . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 615.12 Unpopulated Second Revision Printed Circuit Board . . . . . . . . . . . . . 625.13 Second Order, Three State Breadboard ∆Σ Modulator . . . . . . . . . . . . 635.14 Populated Second Revision Printed Circuit Board . . . . . . . . . . . . . . . 63

6.1 Plot of Efficiency vs. Signal Frequency . . . . . . . . . . . . . . . . . . . . . 686.2 Plot of Efficiency vs. Output Peak Voltage . . . . . . . . . . . . . . . . . . . 696.3 THD results for Loopback Test . . . . . . . . . . . . . . . . . . . . . . . . . 716.4 Frequency Response results for Loopback Test . . . . . . . . . . . . . . . . . 716.5 THD results at 5MHz clock frequency . . . . . . . . . . . . . . . . . . . . . . 726.6 Plot of SNR vs. Frequency . . . . . . . . . . . . . . . . . . . . . . . . . . . . 736.7 Plot of Efficiency vs. Output Peak Voltage . . . . . . . . . . . . . . . . . . . 75

G.1 A preliminary schematic . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 116

H.1 Preliminary Schematic of the Power and Filter Stages . . . . . . . . . . . . . 117H.2 Final Schematic - Modulator . . . . . . . . . . . . . . . . . . . . . . . . . . . 118H.3 Final Schematic - Power Stage and Filter . . . . . . . . . . . . . . . . . . . . 119

L.1 THD results for Loopback Test . . . . . . . . . . . . . . . . . . . . . . . . . 141L.2 Frequency Response results for Loopback Test . . . . . . . . . . . . . . . . . 141L.3 THD results at 1MHz clock frequency . . . . . . . . . . . . . . . . . . . . . . 142L.4 SNR results at 1MHz clock frequency . . . . . . . . . . . . . . . . . . . . . . 142L.5 Frequency Response resuplotlts at 1MHz clock frequency . . . . . . . . . . . 143L.6 THD results at 2MHz clock frequency . . . . . . . . . . . . . . . . . . . . . . 143L.7 SNR results at 2MHz clock frequency . . . . . . . . . . . . . . . . . . . . . . 144L.8 Frequency Response results at 2MHz clock frequency . . . . . . . . . . . . . 144L.9 THD results at 5MHz clock frequency . . . . . . . . . . . . . . . . . . . . . . 145

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L.10 SNR results at 5MHz clock frequency . . . . . . . . . . . . . . . . . . . . . . 145L.11 Frequency Response results at 5MHz clock frequency . . . . . . . . . . . . . 146L.12 THD results at 10MHz clock frequency . . . . . . . . . . . . . . . . . . . . . 146L.13 SNR results at 10MHz clock frequency . . . . . . . . . . . . . . . . . . . . . 147L.14 Frequency Response results at 10MHz clock frequency . . . . . . . . . . . . . 147

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List of Tables

1.1 Project Specifications . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2

2.1 A Comparison of Half-Bridge and Full-Bridge Amplifiers [HA05] . . . . . . . 14

3.1 MOSFET Comparison Table . . . . . . . . . . . . . . . . . . . . . . . . . . . 293.2 The values for the “dummy filter” [TI:99] . . . . . . . . . . . . . . . . . . . . 29

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Executive Summary

The purpose of this project was to design and implement a Class D audio amplifier. Class

D amplifiers improve upon the traditional amplifier design by amplifying a digital signal

instead of an analog signal for drastically superior efficiency. These amplifiers, because of

their efficiency specifications, are often used in portable applications where small size and low

power consumption are important for portability and battery use. This report discusses the

design of a Class D audio amplifier that, at 80 Watts, is powerful enough to facilitate a small

concert while maintaining 90% efficiency for lower energy usage and costs. With the growing

concern regarding the human impact on the environment and increasing energy costs, it is

becoming necessary to design higher power devices more efficiently to reduce environmental

repercussions and improve marketability. The efficiency also removes the need for heat sinks,

which often contribute significantly to the weight of a system, as little power is dissipated in

the amplifier. This increases the portability of the sound system for touring artists or others

who wish to transport audio equipment. While sound quality is often compromised in Class

D audio amplifiers, this system was designed with less than 1% Total Harmonic Distortion

(THD) and with a Signal to Noise Ratio (SNR) of greater than 90dB to provide quality

comparable to Compact Disc (CD) recordings. This project was advised by Professors John

McNeill and Andrew Klein and was possible largely as a result of the generous sponsorship

provided by the NECAMSID Lab.

Class D audio amplifiers achieve impressive efficiency specifications using a technique

that, until recently, was impractical due to component constraints that limited sound quality.

The amplifier functions using a modulator to convert the analog input to a digital signal. This

modulation could be accomplished in a number of ways, provided that the audio signal could

be reconstructed from its digital representation with a filter. Common techniques include

Pulse-Width Modulation (PWM), Delta-Sigma (∆Σ) modulation or the implementation of

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a Digital Signal Processing (DSP) chip. This modulation stage was restrictive until recently

when advancements in Integrated Circuit (IC) design, combined with the use of feedback,

were able to provide a low-noise solution that was practical for audio applications. Once

the modulation stage produces a digital signal, transistors can increase the power in the

digital signal while acting in only the saturation and cutoff regions, thus avoiding the losses

introduced in the linear region. The remarkable efficiency of the Class D amplifier is a result

of this mode of operation. Traditional amplifiers, in contrast, use transistors to directly

amplify audio signals, and are therefore forced to operate in the linear region where the

most losses are incurred. The high-powered digital signal produced by the transistors in

a Class D amplifier is finally applied to a filter. This reconstructs an amplified version of

the original audio signal, removing the noise introduced by the modulator to the frequency

spectrum above the audio band. The filtered signal is then applied to a load, usually a

speaker or a recording device in the case of audio amplifiers.

Extensive research showed that the optimal design for this product would utilize ∆Σ mod-

ulation and an H-Bridge power stage connected to a passive Butterworth filter. Once these

system-level decisions were made, the details of each stage were considered. To maximize

efficiency and quality, the modulator became a three-state, second order modulator. The

three-state operation minimized switching when the input signal approached zero to improve

efficiency and audio quality, and the second order configuration provided better noise shap-

ing which also improved the quality of the output signal. In the power stage, Metal-Oxide

Semiconductor Field Effect Transistor (MOSFET) and MOSFET driver choices became the

most important design decisions. After careful analysis of different MOSFETs, the IRF6645

emerged as the best choice because of its low RDS−on and CGS values. The driver chosen was

designed specifically to work with the IRF6645. With the filter design, components were,

again, the most important factors. The Coilcraft D1787 inductors and polyfilm capacitors

were instrumental in reducing microphonics and unwanted losses in the filter.

This project went through two major design revisions. The first implementation included

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a bread-boarded, first order, modulator and a PCB that contained the power stage and the

filter. This was mainly to ensure the functionality of the design and to find issues with

system implementation. Once the known errors in the initial implementation were rectified,

a final, smaller PCB was created that included space for the modulator as well as the power

stage and filter. Though the modulator on the PCB did not work due to errors in the layout,

a new second order, three state modulator was realized on a breadboard that worked with

the smaller, improved power stage and filter.

The final design was tested extensively to verify that it met the original specifications.

The product was successful in producing output power greater than 80 Watts with an 8Ω

load. The amplifier efficiency was greater than 95% at full output power, the SNR of the

system was above 90dB and the THD was below 1%, as expected.

This design was successful in achieving the goals established at the onset of the project.

All specifications were met and the members of the team learned a great deal throughout the

design process. Taking an idea throughout all the stages of production, including background

research, design, implementation, functionality testing, revision and specification verification,

was an extremely rewarding process. Class D is essential to the future of audio amplification

and environmental sustainability, and this project has demonstrated that the technology can

be applied to higher power systems without diminishing efficiency or audio quality.

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Chapter 1

Introduction

Class D amplification is achieved by modulating a signal, amplifying the modulated signal

and then filtering the amplified signal back into its original form. Since Class D amplifiers

work with digital signals, they do not require that the transistors involved operate in the

triode region and, as a result, they are much more efficient than other amplifiers. This

method has been used in portable audio devices, cell phones and low fidelity audio where

size, power and heat dissipation are of great concern. The advantages of Class D, however,

can also be applied to the larger systems required for live audio.

The purpose of this project was to produce a live audio Class D amplifier. The reduction

in power consumption made possible by a Class D system is sometimes considered unneces-

sary for live audio because the size and efficiency of an audio system is not usually a concern

when the system is permanently installed in a venue and the power is drawn from the wall.

There are traveling musicians, however, who require a more compact system that can be

easily moved from one venue to another. With a more efficient system comes smaller heat

sinks and thus smaller systems that can be portable even if they must be plugged into the

wall. Furthermore, with environmentalism becoming more and more important, especially

among those in the music industry, the advent of audio systems that require less power than

current systems is very attractive. Finally, venues themselves may wish to purchase these

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systems simply to save energy, which is becoming increasingly expensive. These savings may

be significant for venues that have shows every night.

1.1 Project Objectives

This project produced a prototype for a live Class D audio amplifier. The specifications in

Table 1.1 show the specifications that were outlined for this project.

Specification V alueOutput Power (RMS) 80W

Efficiency ¿90%Total Harmonic Distortion (THD) ¡1%

Signal to Noise Ratio (SNR) ¿90dBFrequency Response 3dB from 20Hz to 20kHz

Table 1.1: Project Specifications

1.2 Report Organization

This report follows the progress made throughout this project. In Chapter 2, background

research is presented to prepare the reader for the remainder of the report. Chapter 3 deals

with the preliminary design that led to the first revision of the prototype. The results of the

testing done on this revision are given in Chapter 4. Chapter 5 explains the changes made

to advance the prototype to the final revision. Chapter 6 gives the results from the testing

of the final revision as well as a discussion of how well the product met the specifications

outlined in Section 1.1. Finally, Chapter 7 presents the conclusions reached over the course

of the project and Chapter 8 makes recommendations for future projects in Class D audio

amplification.

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Chapter 2

Background

This chapter discusses the Class D audio amplifier and each of its principal components.

It presents two different possibilities for the modulation stage: Pulse Width Modulation

and Delta Sigma Modulation. It also examines the power stage and explores half- and full-

bridge amplifiers. Filtering is also discussed in this chapter and different types of noise are

investigated.

2.1 Class D Amplification

The Class D amplifier is one of many classes of amplifier. Some other amplifier designs,

like Class A, Class B, and Class AB, are widely used because of their simplicity and ease

of use in almost any application. Class D amplifiers have historically only been used in a

limited number of applications, like motor control, because it is more difficult to generate

the high quality signals required for audio applications with a Class D amplifier. Recently,

however, Class D technology has advanced sufficiently to allow these amplifiers to accurately

and cleanly amplify audio signals. There are many advantages to using Class D amplifiers

for audio applications, and the number of disadvantages is shrinking every year with further

advances in technology.

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2.1.1 Operation of Class D Audio Amplifiers

To understand how a Class D amplifier works, it is important to present the basics for

amplification with a discussion of the Class A amplifier. A Class A amplifier usually uses

a Bipolar Junction Transistor (BJT) to directly amplify an input audio signal. This is a

simple process, involving the input signal, the amplifying BJT, power rails, and the output,

configured as shown in Figure 2.1.

Figure 2.1: A Class A audio amplifier.

The BJT amplifies the signal by operating in the linear region. This allows the output

voltage to vary based upon the principle that the current flowing between the collector and

the emitter of the transistor is proportional to that flowing between the base and the emitter.

As a result, the high power output signal follows the input signal very accurately, reducing

noise and distortion. The linear region of the transistor, however, is very inefficient. It

constantly drains energy from the power supply, even if the input is grounded and there is

no signal to amplify. The maximum theoretical power efficiency of a Class A amplifier is

between 25% and 50%, depending upon the type of output coupling used. This becomes a

problem when an amplifier is used in an audio application because audio is an AC signal and

most of the time the input will be closer to zero volts than it will to one of the rails [Qui93].

For many audio applications, such as home theater or live concert audio, the power efficiency

was not considered until very recently, as there was an “unlimited” amount of power available

when the device was not dependant on a portable energy source. With recent trends towards

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environmentalism, increased energy costs, and higher powered amplifiers, power efficiency is

quickly becoming paramount to the design of audio amplifiers. There are modifications to

Class A, Class B and Class AB amplifiers that increase power efficiency at the expense of

increased distortion, but the maximum theoretical power efficiency is still lower than desired

specifications for this project at 78.5%.

Once the power efficiency specification becomes a top priority, Class D amplifiers become

a more appealing choice. A Class D amplifier is theoretically 100% efficient and can reach

greater than 95% efficiency in practice with current technology [IRF07]. Class D amplifiers

are much more complicated than the other designs that were described, which was a signifi-

cant factor in the preference for other amplifiers until more recent years. Their complexity

can lead to a highly noisy output signal, which made them useless for many applications.

With recent advances in technology, however, the noise can be reduced and then filtered out,

leaving a highly efficient, but still accurate, audio amplifier.

A Class D amplifier has three main stages, the first of which is the modulation stage.

In a Class D amplifier, the signal must be converted to a digital signal before being am-

plified. There are several ways to accomplish this; the two most widely used are Pulse

Width Modulation and Delta-Sigma (∆Σ) Modulation. Each method has advantages and

disadvantages which will be discussed in a later section. After the signal is modulated, it

must be amplified. The amplification stage in a Class D amplifier uses several Metal Oxide

Semiconductor Field Effect Transistors (MOSFETs), a different kind of transistor with very

low power loses. The MOSFETs in a Class D amplifier can switch between fully on and

fully off because they are amplifying a digital signal, avoiding the triode region where power

efficiencies drop. When completely on in the active region, or completely off in the cutoff

region, MOSFETs are theoretically lossless and in practice have very low power losses. After

the modulated signal is amplified, it must be filtered before it can be sent to a speaker. The

last stage is the filtering, or demodulation, stage, which consists of a low pass filter. This

allows everything in the audible range (20 Hz - 20 KHz) to pass through, but significantly

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attenuates everything above 20 KHz. After being filtered, the signal is an amplified replica

of the original input signal, and can be applied directly to a speaker. Figure 2.2 shows how

these blocks fit together.

Figure 2.2: Block Diagram of a Class D Amplifier

2.1.2 Advantages and Disadvantages of Class D

Class D amplifiers have several advantages over Class A, AB, and B amplifiers. The biggest

advantage is the increased power efficiency. A Class D amplifier can reach theoretical power

efficiencies of 100%, and over 95% in actual applications. This is a significant improvement

over the Class B amplifier, which has a maximum efficiency of 78.5%. In high power ap-

plications even a small difference in efficiency is considerable because it allows for a large

reduction in the amount of waste heat generated by the amplifier. Another benefit to Class

D amplifiers is that for lower power applications, they can be fit entirely on an integrated

circuit. For higher power applications a heat sink may be required, but the size of the heat

sink would be much smaller than on a Class A, AB, or B amplifier of comparable power

output. The reduced size of the amplifier leads to lower costs associated with enclosures

for the amplifier. In addition, while the amplifier design itself is more complicated, many

of the internal components, such as the MOSFETs, integrated circuits, and capacitors, are

extremely cheap when purchased in bulk.

While Class D amplifiers have been in use for many years, only recently have they come

to the forefront of audio amplification. This is because Class D amplifiers have a number of

disadvantages that make them less suitable for audio amplification, though many of these

have been overcome with recent advances in technology.

One major disadvantage is that a Class D amplifier has a very high amount of high

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frequency noise, generated by the switching design [Qui93]. This noise must be kept at a

high enough frequency to be inaudible, yet to a minimum amplitude to meet FCC regulations.

To help reduce extraneous noise, a filter is added after the amplifying stage. This filter is an

additional component of the Class D amplifier, and adds complexity, weight, and cost. The

added weight is negligible, however, when compared to the weight of the heat sink required

for a Class A, Class AB or Class B amplifier. The additional cost of a filter may also be

minimized using careful design techniques. Since the filter only needs to attenuate signals

above the audible frequencies, it is not essential that the filter be extremely precise. The

filter may therefore be realized by a fairly simple, low-pass, passive filter.

A second deficiency of Class D amplifiers is the increased complexity in design. This

may result in increased design time and expense. Increased design expenses are generally

considered acceptable, however, if the result is a lower manufacturing cost because design

is singular expense, whereas manufacturing expenses are recurring. After the amplifier is

designed, most of the components, with the possible exception of any inductors used in

the filter and specialized MOSFETs in the power stage, are extremely inexpensive when

purchased in bulk. So while the increased complexity seems like a major disadvantage, it

may become irrelevant when the amplifiers are mass-produced.

The last major disadvantage of Class D amplifiers is that historically, distortion has been

a major problem. High Total Harmonic Distortion (THD) is indicative of high noise levels,

which detract significantly from the audio quality of the output. Advances in technology

have allowed for faster modulation techniques, however, which can reduce THD to fractions

of a percentage in Class D audio amplifiers.

2.1.3 Applying Class D to Audio Design

High power efficiency, combined with a compact and lightweight design, distinguishes Class D

amplifiers from other amplification techniques. Power efficiency is becoming very important,

as concerns regarding power usage increase. A tangible benefit of reduced power consumption

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is that it becomes less expensive to use the amplifier. While this may not be a major concern

for homeowners, in the live audio market power is sometimes generated on site, especially

for large concerts, and larger generators are more expensive to use. From a marketing

standpoint, the compact and lightweight design made possible by high efficiency is attractive

to all users. Home audio systems can be designed to be hidden away, helping to reduce

clutter in a room. In the touring market, smaller amplifiers mean lower shipping costs and

a reduction in labor when setting up before and packing up after a concert.

2.2 The Modulation Stage

The modulation stage of an analog Class D audio amplifier is primarily influential within

the system in that it drastically affects the quality of the output. The modulation stage

is the first stage in the amplifier, other than the input channel over which the system has

little control. Any information in the original signal that is lost during modulation, either by

attenuation or the introduction of excessive noise, will create distortion in the final analog

output and will decrease the maximum sound quality that is possible at the output.

There are a wide variety of modulation techniques which may be considered for use in

a Class D audio amplifier. Some, however, are more reasonable than others for reasons of

simplicity, effectiveness, and availability for commercial use. Simplicity must be considered

because a simpler design will have fewer components and be lighter and more portable,

thereby increasing its appeal in the live audio market. Effectiveness must also be considered

because modulation is essential to sound quality and the amplifier must achieve less than 1%

distortion and greater than 90dB Signal to Noise Ratio (SNR). The modulation technique

is also limited by availability for commercial use, as it would be impractical to implement a

proprietary modulation scheme or a technique with similar limitations, in the development of

an independent product. With these limitations, the most feasible options are Pulse Width

Modulation (PWM) and Delta Sigma Modulation (∆Σ) [Dal97].

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2.2.1 Pulse Width Modulation (PWM)

Pulse Width Modulation is a technique that represents the amplitude of the input signal

using the duty cycle of the output signal, which is usually bi- or tri-state. While there are

many ways to achieve this, one of the simplest is to compare the analog input signal to a

ramp signal or a triangle wave of a frequency that is at least twice that of the analog input, in

accordance with the Nyquist-Shannon sampling theorem. The resulting output will consist

of a digital signal that contains a logic high whenever the analog signal is higher than the

triangle wave, and a logic low when it is not. This creates a signal with a duty cycle that

represents the instantaneous voltage of the analog input signal [Ber03].

While very simple, available for commercial use, and even somewhat effective, PWM sys-

tems are, in some ways, restrictive. PWM is commonly demodulated using a low pass filter.

The noise spectrum, while having a higher SNR than other types of modulation contains a

large amount of high amplitude noise contained in a series of very narrow frequency bands.

This makes the noise more difficult to remove with filters than if the noise were of equal or

even higher energy, but were spread evenly over a larger number of frequencies. Systems that

contain PWM are also limited in how they can be modified if theory and practice should

differ in the physical implementation of the system. The frequency or amplitude of the tri-

angle wave may be modified, but without adding feedback to the system, it is very difficult

to modify the response of the modulator. Adding feedback provides the system with greater

flexibility regarding any modifications that may be required; however, it also distributes a

greater number of the frequency bands containing high amplitude noise in lower frequencies,

closer to those contained in the analog input signal. This increases the complexity of the

necessary demodulation filters. If a simple system were required and sound quality were not

a priority, pulse width modulation would be a highly effective choice. A slightly more com-

plex modulation technique may, however, provide a significant increase in sound quality and

reduce the minimum distortion to below 1% without incredibly complicated filters, making

it a more optimal choice for this particular system [Max06].

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2.2.2 Delta Sigma Modulation (∆Σ)

∆Σ is another modulation technique that may be realized with a circuit that requires only an

integrator and a D-latch. In this implementation, the input audio signal serves as the input

to a simple integrator circuit. When this signal surpasses a threshold, it resets the integrator

and triggers the D-latch, so that it outputs a pulse of a set width. This provides a series

of set-width pulses with variable spacing between them, whose time-density distribution

represents the instantaneous amplitude of the original input signal.

∆Σ separates itself from PWM by its inherent use of feedback to create a system with

superior noise performance. A system model of a ∆Σ modulator, showing this feedback, is

displayed in Figure 2.3.

Figure 2.3: A system model of a first order ∆Σ Modulator.

The quantizer in this figure poses a problem, however, when attempts are made to model

or simulate this modulator because it is a non-linear component. It is therefore replaced

with additive quantization noise, as shown in Figure 2.4.

Figure 2.4: A system model of a first order ∆Σ Modulator after the quantizer is replacedwith additive quantization noise for modelling and simulation.

Analysis of this system provides Equation 2.1.

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VOUT = (VIN − VOUT )1

sτ+ ǫ (2.1)

Solving for VOUT produces Equation 2.2.

VOUT = [1

1 + sτ]VIN + [

1 + sτ]ǫ (2.2)

This equation contains a signal transfer function and a noise transfer function for the

modulator. These transfer functions produce a graph of the shape shown in Figure 2.5 with

the signal transfer function shown in red and the noise transfer function shown in blue.

Figure 2.5: An approximate representation of the signal (red) and noise (blue) transferfunctions of a simple delta sigma modulator.

In an audio application, it would be ideal for the signal transfer function to be as flat

as possible throughout the audio band and for the noise transfer function to push the noise

as far out of the audio band as possible. The specifics of the transfer functions depend

on the coefficient of integration for the integrator. The feedback may also be scaled to

further affect the transfer function. The order of the modulator may also be increased by

adding integrators and levels of feedback. This increases the slope of the transfer functions.

In an audio application this noise shaping may improve sound quality by decreasing the

amount of quantization noise in the audio band. The modulation frequency also affects the

system by determining the placement of the transfer function in the frequency domain. A

higher modulation frequency will push the noise up to higher frequencies, further reducing

its presence in the audio band.

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Like with the PWM system, the output of a ∆Σ modulator may be demodulated with a

low pass filter. The ∆Σ system, however, has fewer bands with very high noise amplitudes

and generally produces a smoother waveform due to noise shaping. The noise floor in the

audio band is considerably lower than that of the PWM system. Also, when both are

simulated with a modulation frequency that is two orders of magnitude above the highest

signal frequency, the noise reaches a maximum point in PWM systems that is not reached

in ∆Σ systems until a frequency that is two orders of magnitude higher than that in the

PWM system. The ∆Σ system also responds extremely well to feedback, unlike PWM. This

is an important quality because it allows the system to respond to any changes in load that

it might experience, as well as allowing for an improved SNR. ∆Σ is therefore extremely

effective, has a lower SNR than PWM in the audio band, as well as in other, lower frequency

bands. It is also extremely simple to implement and is commercially available, making it a

solution that is close to ideal [Dal97].

2.3 The Power Stage

After the signal passes through modulator, it must be amplified. There are a variety of

methods that can be used to amplify a modulated signal. Most Class D systems use either

a half-bridge configuration or an H-bridge (full-bridge) configuration. No matter what the

configuration, the main components of the amplifier are MOSFETs that are powered by

drivers designed for that purpose. This is why the Class D amplifier is so efficient. The

transistors do not have to operate in the triode region because they are amplifying a digital

signal.

2.3.1 Half-Bridge Amplifiers

One configuration of the power stage is the half-bridge amplifier. Figure 2.6 shows the

schematic for a basic half-bridge amplifier. In this configuration, two MOSFETs are used

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and either one or the other is turned on. Each of these MOSFETs exposes the load resistor to

either a positive or negative rail. This design is very simple and requires very few components.

Figure 2.6: A Half-Bridge Amplifier

2.3.2 H-Bridge Amplifiers

Another common configuration is the H-bridge or full-bridge amplifier. Figure 2.7 shows the

schematic of a full-bridge amplifier.

Figure 2.7: An H-Bridge Amplifier

A full bridge amplifier always has two of the four MOSFETs on at a time. This differs

from the half-bridge amplifier, which has only two possible states, in that the full bridge can

achieve three different states. The states are positive, negative and neutral. The amplifier

gives the load a positive voltage when switches AH and BL are on at the same time, a

negative voltage when BH and AL are on, and the load is grounded when AL and BL are

on at the same time. When using an H-bridge it is extremely important to make sure that

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AH and AL are never on at the same time and that BH and BL are never on at the same

time because this would short the rails and damage both the amplifier and the speaker.

2.3.3 A Critical Evaluation of Half- and H-Bridge Amplifiers

There are advantages and disadvantages to each of the different amplifier designs. Table 2.1,

taken from an International Rectifier application note [HA05], outlines the clear advantages

and disadvantages of each with respect to Class D amplification. This table shows that the

main problem with a full bridge is that there are more components. Additional MOSFETs

and drivers are necessary. The advantages far outweigh the disadvantages, however. Two

of the big advantages of the full-bridge are that even order harmonic distortion and DC

offsets are canceled out, which is extremely important in audio systems. Harmonic distortion

negatively affects the quality of the output and DC offsets can damage a speaker. Removing

this harmful DC offset in a half-bridge amplifier would require using a more complicated

power conditioning stage. This application note goes on to say that, “a full-bridge is better

in audio performance . . . a full-bridge topology allows of the use of a better . . .modulation

scheme, such as three-level PWM” [HA05], thus increasing the capability of the amplifier.

Half-Bridge vs. Full Bridge

Half-Bridge Full-BridgeSupply Voltage 0.5 x 2ch. 1Current Ratings 1 2

MOSFETs 2 MOSFETs/CH 4 MOSFETs/CHGate Driver 1 Gate Driver/CH 2 Gate Drivers/CHLinearity Even and Odd Order HD No Even Order HDDC Offset Adjustment is needed Can be canceled out

Modulation Pattern 2 level 3 level can be implemented

Table 2.1: A Comparison of Half-Bridge and Full-Bridge Amplifiers [HA05]

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2.3.4 MOSFET Drivers

A MOSFET gate may be modeled as a small capacitor that must be charged for the MOSFET

to turn on. The voltage across the gate must be at least 5 volts higher than the drain voltage

for the MOSFET to turn on. For Class D audio amplifiers, the MOSFET between the high

voltage rail and the load must be referenced to the high voltage rail. This is a problem

because the modulator output will be at the low voltage levels used in logic circuits. To

resolve this issue, a MOSFET driver must be used to convert the low voltage level to the

higher voltage required, as well as to provide a higher current to more quickly change the

voltage of the gate of the MOSFET. Additionally, using a driver will more easily allow for

controlling the “dead time”, or the small delay in turn on times. This helps to prevent

shoot-through as well as to reduce total harmonic distortion.

2.4 Noise and the Filtering Stage

The output of the amplifying stage must be filtered before reaching the speaker because the

signal is a modulated pulse wave, not an analog audio signal that can serve as an output to

the speaker. The image shown in Figure 2.8 displays a 2kHz signal modulated at 10MHz

using the Matlab code found in Appendix A. This represents a typical output from a

delta sigma modulator in the frequency domain, although depending upon the modulation

frequency the noise response may be shifted up or down in frequency.

The 2kHz signal is evident, but there is a significant amount of noise surrounding it that

needs to be filtered out. There are a number of ways to filter out the noise, and it can

be categorized into several different types of noise. The following section of this document

discusses noise and the different filters available to attenuate it.

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103

104

105

106

−20

0

20

40

60

80

100

120

Frequency (Hz)

Am

plitu

de (

dB)

Delta Sigma Modulated Signal

Figure 2.8: A 2kHz signal modulated at 10MHz with delta sigma modulation.

2.4.1 Types of Noise

One of the easiest ways to determine the quality of any amplifier is by evaluating the amount

of noise present in the output. This is especially true for audio amplifiers that are noted

for efficiency, as noise will waste power as well as degrading the quality of the signal and

possibly damaging the speaker. Class D amplifiers are extremely susceptible to noise, as

the modulation of the signal adds noise to the system. While it is easy to identify that the

presence of excessive noise will degrade the audio quality of the system, there are actually

several different types of noise, each with their own characteristics. To actively compete in

the audio amplifier market, any new amplifier design must have impressive specifications

regarding two different types of noise: general noise which is represented by the Signal to

Noise Ratio (SNR) of the output, and harmonic noise, which is evaluated using the Spurious

Free Dynamic Range (SFDR) standard. The latter is related to Total Harmonic Distortion

(THD) which is a much more commonly understood specification. While the influence of

SFDR on a system is not recognized by many marketing professionals and purchasers of

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audio amplifiers, its relationship to the more common specification allows it to contribute to

the marketability of an amplifier.

Signal to Noise Ratio (SNR)

A Signal to Noise Ratio is a parameter that describes the ratio of the signal power to the

noise power in a system. In the application of audio amplifiers, the output SNR is measured

on the output of the filtering stage and is considered to be the ratio of the final amplified

signal power to the final amplified noise power. THD is excluded from this noise power

measurement because it is specified separately. For audio signals, this ratio is represented in

decibels (dB), and can be calculated using Formula 2.3.

SNR = 10 logPsignal

Pnoise

(2.3)

In general, the SNR measures the difference between the audio signal and the noise

floor. The noise in the noise floor contains several different types of noise that can sum to

create an audible “hiss” in high power applications. For the most part, it is impossible to

eliminate this background nose entirely by conventional means, although it can be reduced

significantly with careful design. One cause of noise is thermal excitation in the amplifier.

While MOSFETs are generally very accurate, there can be random thermal excitation in the

silicon, which may cause a small current to flow when none is desired. Similarly, if there is

any sort of background noise in the input signal, it will be amplified and will contribute to

the system noise floor, reducing the SNR. It is therefore important to have an SNR that is

as high as possible, because a higher SNR allows for a higher quality output.

Spurious Free Dynamic Range (SFDR) and Total Harmonic Distortion (THD)

Spurious Free Dynamic Range (SFDR) is an important specification in amplifier design.

It is usually used in reference to analog to digital converters (ADC) and digital to analog

converters (DAC) but because ∆Σ modulation, an ADC technique, is implemented in the

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modulation stage, SFDR may be considered. The SFDR refers to the ratio between the

desired signal and the highest amplitude spurious, or unwanted, signal. The spurious signal

does not need to be a harmonic of the fundamental signal, but in many cases it will be. If

the spurious signal is a harmonic of the fundamental frequency, then it will be a portion of

the Total Harmonic Distortion (THD). THD is a ratio of the fundamental frequency to the

sum of the harmonics, though in practice anything more than the fifth harmonic usually will

not contribute significantly to the THD.

Both SFDR and THD can be caused by several different problems in the system. One

such example is clipping of the audio signal. The modulator is designed to support signals up

to a certain amplitude. At that amplitude, the modulator outputs a signal that is a constant

logic high. The filter will then be designed such that at that amplitude, the output signal

will also have a known amplitude. For any input values higher than the system can support,

the output signal will have the same known amplitude that it does when the input value

is exactly as high as the system can support. The information that represents the exact

amplitude will therefore be lost, and the system will only indicate that the amplitude is at

or above a threshold. Fortunately, this is easy to avoid by carefully monitoring input levels

to ensure that the input stays within the correct range. Another issue that may decrease

SFDR and THD values is non-linearity in the amplifier. Class A amplifiers are known for

their exceptional linearity, but they are also notoriously inefficient. Class AB amplifiers are

a compromise, sacrificing some linearity for a higher power efficiency. Class D amplifiers

are more complicated, however. Acceptable linearity can be achieved, but that linearity is

dependent upon modulation technique and filter quality. Even if the amplifier is not perfectly

linear, a filter may be able to help reduce spurious noise if it is above the audible band of

frequencies.

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2.4.2 Passive Filters vs. Active Filters

The first decision in filter design is determining whether to use a passive or active filter.

Passive filters are made up of powerless or passive components like resistors, capacitors and

inductors. An active filter contains one or more powered components, usually operational

amplifiers. This allows for the addition of gain to the filter and allows the filter to be more

accurate. Figures 2.9 and 2.10 show simple schematics of an active low-pass filter and a

passive low-pass filter, respectively.

Figure 2.9: A basic active low pass filter.

Figure 2.10: A basic passive low pass filter.

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The components in each design that introduce complexities into the system are the op-

amp in the active filter and the inductor in the passive filter. The difficulty with op-amps

is that they require external power and are limited in what frequencies they can handle

[Lac91]. Inductors, on the other hand, are difficult to tune accurately and are can be bigger

and more expensive than op-amps [Lac91]. Active and passive filters also differ in that an

active filter contains resistors and an op-amp which introduce losses, whereas a passive filter

can be realized with just inductors and capacitors, which have very low losses associated with

them. This is significant because of the efficiency specification for this project. Because of

the nature of the noise that must be eliminated, as shown in Figure 2.8, the cutoff frequency

has no need to be extremely accurate. Most of the noise that must be removed is outside

the audio band, and as long as the filter attenuates most of the noise above the audio band

and not the signal in the audio band, it will be effective. Therefore the benefits of a passive

filter outweigh the disadvantages for Class D audio amplification.

2.4.3 Single Ended Filters vs. Balanced Filters

Choosing a passive or active filter is merely the first step in filter design. There are multiple

configurations within either of those subsets. Once the configuration is chosen, the order of

the filter and the values for each of the components required in the filter must be determined.

The first filter consideration is whether to filter just on one side of the signal with a single-

ended filter, or both sides, with a balanced filter. Figure 2.11 shows the difference in design

of the two filters.

The only advantage to using the single ended design is that there are fewer components.

For Class D, however, using a balanced filter is desirable because it eliminates the DC offset

by centering the signal around zero without the use of a negative rail [TI:99].

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Figure 2.11: Single Ended and Balanced Filter [McD01]

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Chapter 3

Preliminary Design

The following section outlines the design of the preliminary stage of the Class D audio ampli-

fier. This iteration of the design included a bread-boarded first order modulator connected

to a PCB that contained the power stage and the filter. It was known that this design was

not likely to meet the specifications described in Section 1.1. It was, however, important to

make an iteration of the amplifier early on to demonstrate that the design was functional

and test for unforeseen problems that may not appear in simulation. The sections in this

chapter describe how each stage was created, discussing layout and component decisions as

well as the initial PCB and breadboard construction.

3.1 The Modulation Stage

The first step in designing the modulation stage of the system was to determine what mod-

ulation scheme was to be used. Delta Sigma Modulation was chosen because of the superior

noise response and the use of feedback, as explained in Section 2.2.2. Once this was decided

it was possible to design and implement a simulation in Matlab.

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3.1.1 The First Order Delta Sigma Modulator Design

The first system that was simulated and constructed was the first order delta sigma modu-

lator. The simulation itself was based on the schematic shown in Figure 3.1, and the code

was designed to represent the physical system as closely as possible.

Figure 3.1: The schematic used to simulate a first order delta sigma modulator.

The input signal used to test the system was a sine wave that was biased so that the

entire wave was below zero volts. R1 and R2 were both set to 100KΩ, C was set to 0.01µF ,

VQout was represented by 4.9V, and Vthres was 4.2V. These values were taken from data sheets

of actual components and from the idea of a physical system.

Feedback plays a large role in the functionality of this circuit. The operational amplifier

(op amp) is configured to integrate an input voltage using the capacitor, C, in the feedback

loop in conjunction with R1 and R2. The feedback also implies that the voltage on the input

and output terminals is the same, as with many op amp circuits. This property, combined

with the fact that negligible current can flow into or out of the input terminals of the op

amp, allows the op amp to simultaneously be used as a summing amplifier. This provides

the opportunity for another level of feedback, this time from the output of the flip-flop.

The input of the circuit has been biased so that the entire signal is below zero volts and

the voltage on the negative terminal of the op amp is held at zero volts. This causes a current

to flow across R1 towards the input, drawing current through C. When the input signal has

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a higher amplitude it will actually have a lower absolute voltage, causing the voltage drop

across R1, and therefore the resulting current, to be smaller. The feedback from the flip-flop

has the opposite effect. Because the output from the flip flop ranges from zero to five volts,

when the output signal on Q is high, the voltage on Q is low (0V) and has no effect on

the summer. When the output signal on Q is low, however, the voltage on Q is high (5V),

and generates a current that flows from Q to the negative terminal of the op amp that is

larger than the current drawn by the input. This nullifies any effect that the negative input

voltage would have, and pushes a current through the capacitor from the negative terminal

to the output. This resets the integrator, allowing for the removal of the resistor in the usual

parallel capacitor and resistor combination seen in most integrator circuits. It also acts as

an adjustable feedback that can be altered by changing the value of R2. The result is a

modulator with a well behaved noise response and a digital, two-state output that can be

filtered with a simple low-pass filter to reconstruct the original signal.

The Matlab simulation that was based on this circuit is available in Appendix A. The

results of the simulation can be seen in Figure 3.2. They are significant because of the

modulation frequency and the SNR with respect to the signal and the noise floor in the

audio band. The modulation frequency is approximately accurate. With the MOSFETs

that will be used, the maximum modulation frequency possible is likely to be 1MHz to

optimize efficiency. Because the SNR improves with an increased modulation frequency,

and 1MHz is the maximum modulation frequency, the SNR in the audio band is at its

maximum for this modulator at approximately 50dB. This is unacceptable because the SNR

specification for the project is 100dB. Since the modulation frequency cannot be increased

without compromising efficiency, it seems that the optimal solution is to increase the order of

the modulator. For this reason, a second order delta sigma modulator will be implemented.

24

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102

103

104

105

106

107

108

−60

−40

−20

0

20

40

60

80

100

120

Frequency (Hz)

Am

plitu

de (

dB)

Delta Sigma Modulation

Figure 3.2: The results of the first order delta sigma simulation, conducted with a 2kHz sinewave and a 1MHz modulation frequency.

25

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3.2 The Power Stage

The design of the power stage was important for the amplifier to meet the 90% efficiency

specification. Both the configuration of the amplifier and the decision of which MOSFETs

to use were key in reaching this goal.

3.2.1 Amplifier Configuration

As discussed in Section 2.3 of this document, there are two different amplification config-

urations that are used in Class D systems. These are the H-Bridge and the Half-Bridge.

Table 2.1 shows a comparison of these systems that demonstrates that an H-Bridge would

be a much better configuration for this application. Essentially, the H-Bridge eliminates

DC offsets and only requires one power rail. Further, it allows for the possibility of using

three-state modulation, which would increase the efficiency of the system.

3.2.2 MOSFET Selection

The choice of MOSFET is a significant factor in whether or not the amplifier will meet

its efficiency specification. The most important characteristics of the MOSFET in this

application are the peak drain-source voltage it can handle, the resistance in the drain-

source (RDS−on), the gate capacitance (CGS), the time it takes to turn on and off (trise and

tfall) and the voltage required to drive it.

Peak Voltage

Since the system must be able to handle an average of 80 Watts, it must be designed to

survive peaks of up to 160 Watts. The resulting peak voltage can be therefore be found

using the following equations.

R = 8Ω and

P = 160 watts

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P =V 2

Peak−RMS

R

VPeak−RMS =√

PR

VPeak−RMS =√

8 · 160

VPeak−RMS = 35.8V

VPeak = VPeak−RMS ·

2

VPeak = 50.6V

Based on this, the MOSFET must be able to handle a 50V rail in order to be considered.

Loss Terms

The losses in the MOSFETs are mainly a result of two different terms. The first is the

RDS−on loss term that describes the losses when the MOSFET is on. This is caused by an

equivalent resistance in the switch. The equation for RDS−on losses is shown in Equation 3.1.

PDResistive = I2out · RDS−on (3.1)

In the worst-case scenario there would be 40VRMS across an 8Ω load that would produce

a current output of 5ARMS . The final equation for resistive power dissipation is therefore:

PDResistive = 25 · RDS−on (3.2)

In addition to these resistive losses, there are losses associated with switching. These are

a result of the gate capacitance of the MOSFET, which implies that the gate must charge

up when there is a voltage applied to it. This determines the rise and fall times. A general

timing diagram of how a MOSFET works is shown in Figure 3.2.2.

These losses can be calculated using the following equations. The derivation for these

equations is included in Appendix D:

PDSwitching = (trise + tfall) ·VDD

RLoad

· fsw (3.3)

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Figure 3.3: A MOSFET timing diagram.

PDCGS= fsw · CGS · VDrive (3.4)

Note: In these equations fsw is the switching frequency of the MOSFET, VDrive is the

driving voltage of the MOSFET, Iout is the output current from the MOSFET, and VDD is

the voltage across the MOSFET.

There are also some important loss equations that depend on the filter. The derivations

for these equations are also given in Appendix D. They will become increasingly impor-

tant when deciding which filter components to choose, but also play an important part in

determining how the system will interact with different MOSFETs.

PDF ilterInductor =V 2

DD · rL

192 · L2 · f 2sw

(3.5)

PDF ilterCapacitor =V 2

DD

192 · rC · R2Load · C

2 · f 2sw

(3.6)

Using these equations and the loss equation for resistive power dissipation, the total losses

for a MOSFET at a given frequency can be determined.

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Comparison Chart

The MOSFETs in Table 3.1 were considered because they met the peak voltage requirement

and had relatively low drain-source resistance and gate capacitance.

Part Number Peak Voltage RDS−on CGS trise tfall PriceIRF1010EZ 60V 8.5 mΩ 2810 pF 90 ns 54 ns 4.80IRF3805 75V 3.3 mΩ 7960 pF 150 ns 93 ns 6.48IRF3808 75V 7.0 mΩ 5310 pF 140 ns 120 ns 4.11IRF1405 55V 4.9 mΩ 4780 pF 110 ns 82 ns 5.35IRF3205 55V 6.5 mΩ 3450 pF 95 ns 67 ns 3.34IRF6645 100V 28 mΩ 890 pF 5 ns 5.1 ns 2.98IRF6665 100V 53 mΩ 530 pF 2.8 ns 4.3 ns 2.98

Table 3.1: MOSFET Comparison Table

Based on the values in Table 3.1 and the equations above, the losses for each MOSFET were

calculated. In order to do this, a “dummy filter”, based on the values in Table 3.2, was

applied [TI:99]. Combining all the loss terms, the curves in Figure 3.4 were produced to

compare the different MOSFETs to see which ones would incur the lowest losses.

DC Load Resistance Cutoff Frequency Inductor Value Capacitor Value(RL − Ω) (fC − kHz) (L − µH) (CL − µF )

4 20 22.5 1.414 25 18 1.134 30 15 0.944 35 12.9 0.808 20 45 0.708 25 36 0.568 30 30 0.478 35 26 0.40

Table 3.2: The values for the “dummy filter” [TI:99]

Immediately one MOSFET stands out among the rest. Based on this loss curve, the

IRF6645 MOSFET was used for this project.

29

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104

105

106

107

10−1

100

101

102

103

Switching Frequency (Hz)

Pow

er D

issi

pate

d (W

atts

)MOSFET Comparison Graph

Figure 3.4: The curves for each simulated MOSFET.

3.2.3 MOSFET Drivers

As an International Rectifier MOSFET was chosen for the power stage, it was decided to

use International Rectifier MOSFET drivers to control the MOSFETs. This has several

advantages, most important being that the parts are designed by the manufacturer to work

together. This helped to reduce issues in the design of the power stage, including shoot-

through, which is the biggest concern for the first revision of the power stage. Shoot-through

in an H-Bridge occurs when both MOSFETs on one side turn on at the same time, allowing

a direct path from the high voltage rail to ground. There were several choices of MOSFET

drivers from International Rectifier, each with slightly different features. The most useful

driver was the IRS20124s, which has a user-selectable dead time. Being able to control

the amount of dead time was very useful, and allowed for finer control of total harmonic

distortion and reduce the chance of shoot-through.

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3.3 Filter

As discussed in the Chapter 2, the third stage of a Class D amplifier is the filtering stage.

The switching nature of the Class D amplifier causes it to emit a significant amount of

noise above the audio band. While this noise is shaped by the modulator to be above the

20 KHz upper limit of human hearing, it can still cause problems. The biggest concern

is electromagnetic interference (EMI) in equipment along the path of the cabling from the

amplifier to the speaker. To help mitigate the issues caused by the higher frequency content

of the signal, a low-pass filter must be placed before the final output of the amplifier.

The filter stage is the simplest stage of a Class D audio amplifier. A simple low-pass

filter is all that is required, as the audible band of frequencies can be considered a base band

signal when designing an audio amplifier. Since the power stage is an H-Bridge, the filter

is required to be a balanced filter. This means that there are essentially two separate, but

identical filters on either side of the load. This does increase the cost of the final product,

but it is necessary due to the type of power stage used. The H-Bridge and balanced filter

design help reduce noise in the output by eliminating odd harmonics, which improves the

THD.

While there are a number of different filter types, the nature of audio suggests the use of

a Butterworth filter. A Butterworth filter has a very flat pass-band, important for the fre-

quency response specification of an audio amplifier. The slope of the cutoff of a Butterworth

filter can be easily adjusted by increasing the order of the filter, which is accomplished

by cascading additional inductors and capacitors. Due to the shape and location of the

high frequency noise generated by a ∆Σ modulator it was determined that a second order

Butterworth filter would provide the best cost and efficiency to performance ratio.

Once the order is decided, the two parameters that define a Butterworth filter are the

cutoff frequency and the slope of the cutoff. A second order filter results in a slope of -40

dB/decade, which is sharp enough to reduce the high frequency noise to acceptable levels.

The second parameter, the cutoff frequency, determines the component values that should

31

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be used. For the first filter design, a cutoff frequency of 25 kHz was selected to provide a

slight buffer above the audio band, while still attenuating most of the out-of-band noise.

This allows for some tolerance in filter components, which decreases the cost of the filter.

Once the cutoff frequency and the slope of the cutoff were chosen, it was possible to consider

specific filter components.

3.3.1 Filter Components

The specifications of a Butterworth filter are entirely determined by the value and configu-

ration of the components, in this case the inductors and capacitors. Since a balanced filter

consists of two identical filters, one on either side of the load, it is possible to use a half circuit

model to derive filter component values. The half circuit model is depicted in Figure 3.5.

Figure 3.5: Half circuit model of the second order Butterworth filter.[TI:99]

Equations 3.7, 3.8, and 3.9 were derived using the half model circuit to determine the

filter components.

RH =RL

2(3.7)

CH =1

2πfc

2RH

(3.8)

LH =

2RH

2πfc

(3.9)

Using these equations, discrete filter components were selected.

CH =1

2π · 25kHz ·√

2 · 4Ω= 1.13µF (3.10)

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LH =

2 · 4Ω

2π · 25kHz= 18µH (3.11)

Once ideal component values were chosen, real world components were identified. This

resulted in a problem, as a 1.13 µF is not a standard capacitance. Several ceramic surface

mount capacitors were found with a capacitance of 1.2 µF, but they were prohibitively expen-

sive. However, it was possible to slightly adjust the component values with Equation 3.12,

potentially allowing for a pass-band that was not as flat as desired.

fc =1

2π√

2LHCH

(3.12)

While 1.13 µF is not a standard capacitance, 1 µF is. Using the same cutoff frequency of

25 kHz and a CH of 1 µF it was determined that a 22 µH inductor was required. In addition

to the specific inductance, a low Equivalent Series Resistance (ESR) was required. It was

necessary for the inductor to have a low ESR because it was in series with the speaker, so

all of the power from the amplifier flowed through the inductor. Using an inductor with a

high ESR would have significantly lowered efficiency measurements, which would have been

very undesirable for a Class D amplifier. The ESR of the capacitor was of less importance,

as the desired audio signal went through the load, which was in parallel with, and therefore

unattenuated by, the capacitor. The components chosen for the filter were:

Capacitor - Taiyo Yuden UMK325BJ105KH-T (1 µF)

Inductor - Bourns JW Miller 2305-H-RC (22 µH, 7mΩ)

These components were then placed between the MOSFETs and the load, as depicted in

Figure 3.5. Once these filter components were chosen it was possible to construct the first

amplifier revision.

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3.4 System Implementation

After designing the stages for the first iteration of the Class D Audio Amplifier, the pieces

had to be put together. Since the modulator was not in a final design stage, it was assembled

on a breadboard. The power stage and filter were fabricated on a PCB because of the need

for surface mount parts and the fact that at high frequencies there would have been a

significant amount of noise and signal attenuation with the use of a breadboard, especially

at 100 watts. The following section describes how the designs described in the above sections

were assembled and implemented.

3.4.1 First Order Modulator

The first order modulator was constructed on a breadboard for testing with the power

stage, as well as to prove that the concept was feasible. It was assembled based on the

schematic shown in Figure 3.1. Only through-hole components were used in the assembly of

the modulator. R1 and R2 were both 5% 100KΩ ceramic resistors, C was a 0.01µF ceramic

capacitor, an LM356 was used for the op amp, and the flip-flop was a 74HC74A. The clock

signal for the flip-flop was generated by an ECS 2100 1MHz oscillator. This configuration

can be seen on the bread-board in Figure 3.6.

Figure 3.6: The bread-board containing the modulator shown in the schematic in Figure 3.1.

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3.4.2 PCB Layout for Power Stage and Filter

Since the power stage had specialized surface mount MOSFETs and drivers, the stage had to

be fabricated on a PCB. This was created using the Multisim and Ultiboard software package

from National Instruments. First a schematic was created in Multisim. This schematic is

shown in Appendix G. This was transferred to Ultiboard to begin the process of laying out

a PCB.

In designing the PCB, logical layout was extremely important. Since there was a degree

of uncertainty regarding whether or not the design would work, since none of the team

members had used this particular MOSFET and driver set, it was crucial to leave room for

changes and set up test points to simplify debugging. All of the components aside from the

inductors were surface mount components to avoid cluttering up the board and incurring

excess losses. There were two BNC connectors used as injection points for each side of the

H-Bridge. Either a modulated signal or a square wave and an inverted square wave could

be applied to these inputs to test the functionality of the board.

Figures 3.7 and 3.8 show the evolution of the board.

Figure 3.7: The PCB of the Power Stage without Components

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Figure 3.8: The PCB of the Power Stage with soldered components Components

3.4.3 Full System Assembly

Once the PCB and modulator were constructed, the next step was to assemble the full

system by connecting them. The PCB had already been designed to take two inputs from

any modulator and output to a speaker. Since there were tests to be conducted on the PCB

and uncertainties regarding the functionality of the system, the team decided not to use a

speaker directly for this iteration. An 8Ω resistor was fashioned by wiring up 8 - high-power

1Ω resistors together and screwing them all onto a heat-sink. Figure 3.9 shows this resistor

configuration.

Figure 3.9: The Resistor Used for Testing

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Finally all the parts were in place to begin testing. Figure 3.10 shows the entire system

connected together with all the components in place.

Figure 3.10: The PCB of the Power Stage without Components

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Chapter 4

Preliminary Results

The following section discusses the results obtained from the testing conducted on the design

described in Chapter 3. As stated in that chapter, it was not expected that this design

was going to meet all of the specifications outlined in Section 1.1. The testing for this

iteration was mainly for functionality and to see determine the efficiency and signal quality

performance of the amplifier, despite the known flaws in the initial design. The following

section discusses the results of the tests that demonstrated that this preliminary design was

fully functional.

4.1 Functionality Testing

Testing for functionality was the most important aspect of preliminary testing because the

goal was to make sure the design would amplify an input signal. To do this, testing was con-

ducted on each stage independently and the results were compared to an expected outcome.

Once each stage had passed a unit test for functionality, the whole system was assembled to

determine whether the different stages would interact with each other as expected.

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4.1.1 Modulator Functionality

The modulator, as the first stage, was tested for functionality to determine whether it could

pass a modulated sine wave to the power stage for amplification. A qualitative analysis of

the modulator output indicated that it was functioning as expected. Figure 4.2 shows the

input to the system in yellow on Channel 1 and the output of the modulator in blue on

Channel 2, as captured by the oscilloscope. The output of the modulator has the maximum

number of state-transitions when the input waveform is closer to zero, which was an effect

seen in simulation of the first order modulator, shown in Figure 4.1. Like the simulation,

the output also contains longer pulses, either high or low depending upon the amplitude of

the input, that correspond to the maximum and minimum points of the input. The only

significant difference between the appearance of the simulation and the oscilloscope readings

is the scaling that has been performed on the output of the modulator in the simulation.

This simulated signal was halved in order to match the 2 volts/division setting that was

used on the output of the actual system to allow it to fit on the oscilloscope screen. In the

original simulation, both the input and output signals of the simulation and the oscilloscope

matched in amplitude.

1.45 1.46 1.47 1.48 1.49 1.5 1.51 1.52 1.53 1.54 1.55

x 10−3

−3

−2

−1

0

1

2

Time (s)

Am

plitu

de

First Order Delta Sigma Modulation (10kHz Sine Wave, 1MHz Modulation Frequency)

Figure 4.1: The Matlab simulation of the first order modulator.

Further proof of the functionality of the first order modulator is offered in Section 4.1.4,

39

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Figure 4.2: The output of the first order delta sigma modulator, with a 1MHz modulationfrequency and a 10kHz sine wave.

when the entire system is assembled and the modulator output is fed into the power stage,

and filtered. A quantitative analysis of the modulator as a unit was not performed. This

was because it was already clear from simulations that the first order modulator would not

meet the necessary specifications, and that it would make sense to move to a second order

modulator. The construction of the first order modulator was simply a tool to determine

that the general design was functional and to provide the means for testing the remainder

of the system: the power stage and filter on the PCB.

4.1.2 Power Stage Functionality

Once the power stage was assembled on the PCB, it was necessary to test it before connecting

it to the bread-boarded modulator. Since there were two BNC connectors to serve as inputs

to either side of the H-Bridge, this did not pose any major problems. The first point to check

was whether or not the drivers could produce an output signal. After assembling only the

driver circuit without the MOSFETs, a square wave was applied to the input and the output

was monitored. The driver circuit was proven functional when a square wave was observed

on the high side of the driver that followed the input square wave, along with another square

wave on the negative side of the driver that was an inverted form of the input.

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Once the drivers were working, the MOSFETs were added and the rails on the MOSFETs

were powered to determine whether they were switching based on the signal from the driver.

This test was still conducted one stage at a time. The result was a square wave that followed

the input signal, ranging from 0V to 40V on the output, as expected. Figure 4.3 shows an

example of one of these outputs. In this figure, Channel 1 (yellow) represents the input while

Channels 3 and 4 (purple and green, respectively) represent the driver outputs. Channel 2

(blue) is the full output of the power stage.

Figure 4.3: The Power Stage Output

These tests proved that the drivers and MOSFETs were working correctly.

4.1.3 Filter Functionality

Once the power stage was working it was necessary to test the filter. Because the filter

was a balanced filter designed for an H-bridge, it was extremely difficult to test the filter

independently of the power stage. As a result, the method used to test the filter involved

connecting it to the power stage and applying a square wave on one half of the H-Bridge.

The input to the other half of the H-bridge was supplied by a 74C04 inverter, which applied

the inverse of the original square wave. This was the first time that the full power stage was

in use. Since the filter was to be low-pass with a cutoff frequency of 25kHz, the output was

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expected to vary based on the input frequency. If the frequency of the square wave input

was significantly below the cutoff frequency, enough to allow three or four harmonics to pass

through the filter, then a square wave from -40V to 40V would be the expected output.

This was originally tested by connecting the oscilloscope across the resistor load in the

filter. In this configuration, due to the internal grounding of the oscilloscope, the grounding

loop of the probe was connected to the same ground as the PCB causing the test to fail.

The testing procedure was then modified to use a grounded probe at each end of the resistor

and subtract the two values using the MATH function on the oscilloscope. A picture of this

setup is shown in Figure 4.4.

Figure 4.4: The configuration of the test resistor and the oscilloscope probes.

The Figures 4.5 and 4.6 show some of the results of 1kHz and 10kHz square wave inputs

to the power stage and the filter. Figure 4.5 shows that the 1kHz square wave was applied to

the system, was amplified, and remained unfiltered. This is because it had many harmonics

that were within the pass-band of the filter. In contrast, Figure 4.6 shows that the 10kHz

square wave was amplified but since it only had two harmonics in the pass-band, the output

more closely represented a sine wave than the input did.

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Figure 4.5: The power stage and filter with a 1kHz square wave input

Figure 4.6: The power stage and filter with a 10kHz square wave input.

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4.1.4 System Functionality

Once all the individual tests were completed, the final step was to connect the modulator

to the inputs of the PCB. In this stage of testing, the functionality tests of the modulator

were verified when the system output was filtered. This test indicated that the modulator

was functional because the input waveform was replicated at the output of the filter.

For this functionality test, a sine wave served as the input to the modulator. This input

was offset by -1.5V, for reasons noted in Section 3.1.1. It was determined that if the output

was an amplified version of the input, with some reasonable amount of distortion due to the

known issues with the modulator, then that would prove that the full system was functional.

Figures 4.7 and 4.8 show the outputs of the full system.

Figure 4.7: The full system with a 1kHz sine wave input.

These figures show that the complete system was able to modulate both a 1kHz and

10kHz signal, amplify them, and filter them back out to produce sine waves at the output.

The outputs are noisier than would be desired, but this is because the design was still in its

first revision.

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Figure 4.8: The full system with a 10kHz sine wave input.

4.2 Efficiency Testing

Once it was shown that the filter was completely functional, tests were run to determine

how efficient the first iteration of the system was. It was noted that changing the input

frequency and amplitude would change the efficiency measurements, so this test included

sweeping through a set of frequencies in the audio band and going from a small input signal

to the largest input signal that the system could handle while measuring efficiency. The

efficiency was calculated by taking the input current from the power stage, measured with

digital ammeter, multiplying it by the measured input voltage to get the input power. Then,

the output RMS voltage was measured on the load and that was squared and divided by the

output resistance (8.05Ω) to get the output power.

Efficiency =Pout

Pin

(4.1)

Pin = Vin(DC) · Iin(DC) (4.2)

Pout =V 2

out(RMS)

Rload

(4.3)

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Efficiency =Vin(DC) · Iin(DC)

V 2out(RMS)

Rload

(4.4)

Using this data, various frequencies and amplitudes were tested and the values were

recorded to calculate efficiency. As shown in the plots in Figures 4.9 to 4.13, the efficiency

was above the specification of 90% for some input values but not for others. This was

improved upon in the final design.

101

102

103

104

105

0

10

20

30

40

50

60

70

80

90Plot for Efficiency of Output Signals at Vrms=11.2V

Input Signal Frequency (Hz)

Effi

cien

cy (

%)

Figure 4.9: Efficiency Plot at 11VRMS at the Output

4.3 Frequency Response Testing

The frequency response of the system was also tested on the first iteration of the board.

This test was conducted using the same data as was used in Section 4.2. For these plots,

the gain was calculated by dividing the output RMS voltage by the input RMS voltage (see

Equation 4.5).

Gain =Vout(RMS)

Vin(RMS)

(4.5)

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101

102

103

104

105

0

10

20

30

40

50

60

70

80

90

100Plot for Efficiency of Output Signals at Vrms=25.2V

Input Signal Frequency (Hz)

Effi

cien

cy (

%)

Figure 4.10: Efficiency Plot at 25VRMS at the Output

6 8 10 12 14 16 18 20 22 24 260

10

20

30

40

50

60

70

80

90

100Plot for Efficiency of Input Signals at f=50Hz

Output Signal Amplitude (Vrms)

Effi

cien

cy (

%)

Figure 4.11: Efficiency Plot at 50Hz

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6 8 10 12 14 16 18 20 22 24 260

10

20

30

40

50

60

70

80

90Plot for Efficiency of Input Signals at f=12000Hz

Output Signal Amplitude (Vrms)

Effi

cien

cy (

%)

Figure 4.12: Efficiency Plot at 1200Hz

Contour Efficiency Plot

Input Signal Frequency (Hz)

Oup

ut V

olta

ge (

Vrm

s)

102

103

104

8

10

12

14

16

18

20

22

24

Figure 4.13: Efficiency Plot at all Frequencies and Output Voltages

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101

102

103

104

105

38

40

42

44

46

48

50

52Gain Plots at Different Output Voltages

Input Signal Frequency (Hz)

Gai

n (d

B)

6.658.8911.1613.4515.7818.1618.0922.8325.14

Figure 4.14: Frequency Response Plots

As shown in Figure 4.14, the frequency response was not ideal. The frequency roll-off

began inside the audio band. This was remedied with a change of the cut-off frequency from

25kHz to 30kHz and a recalculation of the filter component values.

4.4 Problems with the Preliminary Design and Tests

There were a number of problems with this design. Some of them were expected and some

were not. It was expected that the output would be fairly noisy since the modulator was

only a first order, two-state modulator, whereas in the final design the modulator was a

second order, three-state modulator. This also explained why the efficiency did not meet the

specification. A few other problems surfaced during the testing phase, however. This section

discusses the different problems discovered. The solutions to these problems are discussed

in Chapter 5.

The first major problem was the instability of the MOSFETs. During normal testing the

MOSFETs would burn out after minimal use. This was fairly difficult to diagnose because

there were a number of reasons for it. One of the major reasons was that it was very

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difficult to solder the IRF6645 MOSFETs because of the unexposed pads on the bottom

of the package. Even when the MOSFETs were adhered to the board, it was difficult to

determine whether or not the leads on the inner pads were actually connected. Another

reason for this failure was that there was some initial testing with the filter stage without a

load resistor. It was later discovered that this could be very harmful to the components in

the power stage because the inductor and capacitor on the filter could store a lot of energy

with no discharge point. This energy could build up and damage the MOSFETs. Another

problem that caused burning out of MOSFETs was the original testing design. Originally

it was thought that the oscilloscope probe could simply be placed across the resistor in the

H-Bridge. The resistor was ungrounded, however, and since the oscilloscope probe grounds

are tied to earth ground, any voltage on the resistor was incorrectly shorted to ground.

Another problem with this design was that the board was “singing” whatever was at

the output. It was later found out that the X7R capacitors were causing problems with

microphonics. In general, the dielectric in an X7R causes physical movement at its operating

frequency. If that frequency is in the audible band and has high enough power, it will be

audible. This can also add distortion to the system. This was fixed by using different

capacitors in the final design.

There was also a problem using the function generator. During the efficiency and fre-

quency response tests, the function generator was set to act like there was a 50Ω load, since

this was the default setting. For this application, however, it was necessary for that setting

to be changed to “High Z”. This was fixed in the test plan for the final iteration.

The final problem was that the filter response was not ideal. It was discovered that there

was a calculation error in the filter design of this stage. This problem and its resolution are

discussed in Section 5.3.

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Chapter 5

Final Design

The preliminary design had many problems which were outlined in Section 4.4. These

problems were all addressed and corrected in the final design of the Class D Audio Amplifier.

Most notably, the modulator stage was changed from a first order, two-state modulator to

a second order, three-state modulator. This chapter explains how these changes were made

to each of the stages and how the final PCB was constructed.

5.1 The Second Order Modulator

The design of the second order modulator differed greatly from the design of the first. Because

the first order modulator was extremely simple, due to its single feedback path, designing a

simulation to match a typical schematic required little preparation. The only components

that could be altered were the input resistor, the feedback resistor, and the capacitor that

affected the constant of integration. A second order modulator typically contains two inte-

grators and either two or three feedback paths, creating stability issues and a need to consider

a number of different feedback paths at once. As a result, it was not immediately feasible

to simulate the second order modulator as a circuit with real resistor and capacitor values.

Developing a system model and determining the coefficients of feedback, the constants of

integration for both integrators, and the coefficients in the signal path made it possible to

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determine how the system would react using more theoretical, and therefore more simple,

methods.

5.1.1 System Model

The system model of a second order delta sigma modulator is developed in Schreier’s

Understanding Delta-Sigma Data Converters, and is shown in Figure 5.1 [ST05]. Using this

model of a second order modulator, the coefficients were determined to adjust the noise

transfer function in Equation 5.1.

QIN = QOUT [−a3 · C3 · s

2− a2 · C2 · C3 · s − a1 · C1 · C2 · C3

s2] + VIN [

B · C1 · C2 · C3

s2] (5.1)

Noise shaping is one of the greatest advantages of delta sigma modulation, and this model

provided an opportunity to optimize the noise transfer function. The feedback coefficients

(a1, a2, a3) were determined, using the Matlab script in Appendix B to be: (a1, a2, a3) =

(49, 4

15, 11

90). The Matlab simulation in Appendix C was then developed to represent the

system model, using the values determined by the a coefficients, and setting B = C1 = C2 =

C3 = 1. B, C1, C3 and C3 were then adjusted to produce the desired noise transfer function.

As shown in the simulation, the final values were (B, C1, C2) = (1/3, 1000000, 1000000). C3

was eliminated because it was determined to equal to one, and therefore had no effect on

the system. C1 and C2 were determined to be equal to the modulation frequency of 1MHz.

It was also determined that for efficiency reasons, the modulator should output a three-level

signal. The simulation reflects this, as the quantizer was developed to have three levels. This

simulation, with these coefficients, produced the results shown in Figure 5.2.

5.1.2 Physical Realization

Once the coefficients were determined, it was necessary to turn the system model into a

physical system. It is important to note that the coefficients could still be adjusted, under

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Layer 1

Figure 5.1: The discrete model of a second order delta sigma modulator [ST05].

102

103

104

105

106

107

108

−150

−100

−50

0

50

100

150

Frequency (Hz)

Am

plitu

de (

dB)

Delta Sigma Modulation (System Model)

Figure 5.2: The results of the system model simulation after adjusting the coefficients.

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the condition that the four terms in the noise transfer function, −a3 ·s2·, −a2 ·C2s, −a1 ·C1·C2

and B · C1 · C2, remained the same. If C1 were halved, for instance, a value of another

coefficient in the third and fourth terms must be doubled to compensate. An approximation

of a physical system was accomplished using a spice package, because it was easier to simulate

a system with real components in a spice package than in Matlab, and it was less expensive

and time-consuming to do so than to use real components. The first step was to develop a

system that would be less than practical to implement, but that served as an intermediate

step between the Matlab simulation and the final implementation of the system. In the

final design, the op amps used as integrators also served as summing amplifiers, integrating

the sum of the input to the integrator and the modulator system feedback. This idea, in

the developmental stages, is complicated by the fact that the resistors that scale the input

and feedback for summing also contribute to the coefficient of integration of the integrator.

In order to simplify the system and allow it to, at first, more directly represent the system

model simulation, an extra summing amplifier was added before each integrator, as shown

in Figure 5.3. Figures 5.4 and 5.5 show the results of the simulation.

Figure 5.3: The intermediate stage between the Matlab simulation of the system modeland the final system.

The final stage was developed by replacing the summing amplifiers, one at a time, with

summing resistors on the integrators and ensuring that the functionality of the system had

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Figure 5.4: The output of the intermediate stage between the Matlab simulation of thesystem model and the final system.

Figure 5.5: The Fast-Fourier Transform (FFT) of the intermediate stage output.

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not changed. The resistor values were determined by first examining the system as a result

of the input, and then as a result of the feedback. Considering one set of summing and

integrator amplifiers, it was assumed, temporarily, that the feedback would be zero. The

voltage output of the summing amplifier would then be a result of the input voltage alone.

That voltage would then be applied to the integrator circuit, and would cause a current

to flow across the input resistor to the integrator. That current was the desired current

contribution to the integrator from the input, and the value for the resistor between the

input and the integrator could be chosen accordingly, as the input voltage range is known.

The process was repeated, assuming temporarily that the input was zero, and the feedback

had a known voltage. The final circuit, with all summing amplifiers removed, is shown in

Figure 5.6.

Figure 5.6: The final spice simulation of the second order delta sigma modulator.

Once the spice simulation was fully functional, the second order modulator was con-

structed on a bread-board, as per the simulation model. As with the first order modulator

bread-board, the assembly involved ceramic capacitors and 5% resistors, LM356 op amps,

and 74HC74A flip-flops. The only new component was the LF311 comparator, used for

the three-level quantizer, as the first order modulator was a two-state system. The bread-

boarded system was fully functional, providing the output shown in Figure 5.7. The success

of the physical modulator indicated that it would be appropriate to include the second order

modulator on the final full-system PCB.

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Figure 5.7: The output of the second order three-level modulator on a bread-board

5.1.3 Modulation Frequency

Once the second order, three-level modulator was realized, it was still necessary to choose

the modulation frequency. There were three factors that played a role in this decision: the

capabilities of the system, sound quality, and efficiency. The capabilities of the system had

to be considered because the components in the modulator would have broken down at

extremely high frequencies. Frequencies this high were never considered, however, so the

limitations of the system did not prove to be a restriction on the modulation frequency.

The next two factors, sound quality and efficiency, had to be considered jointly because

there were specifications to meet for both of them and there would prove to be a slight

trade-off between them. The MOSFETs in the power stage were chosen for their efficiency.

The efficiency was dependant on the switching frequency of the MOSFETs. As shown in

Figure 3.4 the ideal switching frequency of the IRF6645 MOSFET was around 1MHz.

The sound quality, however, was unacceptable at 1MHz as demonstrated in Appendix L,

so higher modulation frequencies were considered. Sound quality proved to meet the 90dB

specification best at 5MHz because a higher modulation frequency pushes more noise out of

the audio band. At 5MHz, it was also demonstrated that the efficiency specification could

be met, as shown in Appendix K. Since there was not a notable difference in sound quality

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between 5MHz and 10MHz and the efficiency was slightly better at 5MHz, that was chosen

as the final modulation frequency of the system.

5.2 The Power Stage

The power stage did not have many problems since it was constructed entirely on a PCB.

The only major change to the power stage was the addition of a larger bypass capacitor near

the 40V rail and tantalum bypass capacitors right near the MOSFETs. This was because

the MOSFETs failed consistently with only a small surface mount capacitor on the rail. The

MOSFETs required dedicated bypass capacitors to store and receive energy from.

Figure 5.8: Addition of Electrolytic Bypass Capacitor at Rails

Figure 5.9: Addition of Tantalum Bypass Capacitor at MOSFET

5.3 Filter

The filter had some major unforeseen issues that needed to be resolved. First, the capacitors

used in the original design produced undesired microphonics that added distortion to the

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system. The choice of a 25 kHz cutoff frequency was also problematic because of non-

idealities in the filter components. Finally, the configuration of the filter was changed to

improve efficiency and cost.

5.3.1 Capacitor Microphonics

One problem was the issue of microphonics in the capacitors. The capacitors originally

used for the filter were X7R surface mount capacitors. These are used in many applications

because of their size and low equivalent series resistance (ESR), but they are subject to

microphonics. This means that they emit audible noise at the frequency applied across the

capacitor, so if there is a 1kHz sine wave that is large enough across the capacitor, a 1kHz

tone will be heard. This will decrease the sound quality of the amplifier.

To correct this problem, research on different capacitor types was conducted. This was

a very difficult decision to make because of the vast number of capacitor types. It was

important to choose a capacitor that was free of significant microphonics but that still had

a low ESR to make sure efficiency was still maintained. Polycarbonate film capacitors met

these two specifications and were used in the final design.

5.3.2 Cut-Off Frequency

The frequency response, as shown in Figure 4.14, attenuated more than was desired within

the audio band. This was a result of the fact that the filter used real components whose values

had to be relatively common, so the cut-off frequency ended up being lower than desired. This

was corrected by using a cut-off frequency of 30kHz instead of 25kHz. Increasing the cutoff

frequency had a negligible impact on the performance of the amplifier and ensured there was

no information lost within the audio band. Anything being developed on a commercial scale

must, however, ensure a cutoff frequency of 30kHz is low enough to prevent Electromagnetic

Interference (EMI) to meet Federal Communications Commission (FCC) requirements.

Changing the cut-off frequency necessarily changed the component values. The new value

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for the inductor was determined to be 33µH using Table 3.2. The values for the capacitors

will be discussed in Section 5.3.4.

5.3.3 New Inductors

In searching for new components for the filter, the Coilcraft DL1787 was found. This inductor

improved the efficiency of the amplifier because it had a much lower resistance of 0.0028Ω.

This inductor was also less expensive than the original.

5.3.4 Filter Configuration

The most significant change to the filter was the change in configuration. In the preliminary

design there were two capacitors connected to ground from each end of the resistors (See

Figure 5.10). It was determined that instead, there could be one capacitor across the resistor

with half the value to give the same effect. This decreases both the losses and the cost of the

filter. It was still essential, however, to have some capacitance connected to ground, but these

were much less significant, allowing them to be one tenth the value of what the capacitors

would have been in the old configuration. See Figure 5.11 for the new configuration.

Figure 5.10: Preliminary Filter Design

The values, therefore, of the capacitors were finally calculated to be CL = .47µF and

C = .1µF

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Figure 5.11: Final Filter Design

5.4 Final PCB Layout

Now that the final blocks were all designed, all that was left was to put it all together on one

PCB layout. Since this was to be the final layout, size was a major factor in the design. Each

stage was laid out with the smallest footprint possible. The final PCB, which included the

modulator, power stage, filter, power receptacles and input and output receptacles measured

4.24 inches by 3.05 inches. This was a vast improvement over the previous PCB that was

more twice that size and did not contain a modulator.

Another improvement to the final PCB was the addition of test points throughout the

PCB. The board was laid out so that testing would be very easy for functionality, efficiency

and signal quality. In addition to test points, jumpers and headers were included between

stages, to allow for unit testing. In the preliminary design the modulator and power stage

were separated and had to be connected to work together. This was beneficial because they

could be tested independently of each other; it did, however, make the board a significantly

larger. In the new design there were jumpers in between the modulator and power stage,

as well as between the power stage and filter. Figure 5.12 shows the second revision of the

PCB before it was assembled.

When the PCB arrived, the first section to be populated was the modulator. While

performing functionality tests on the PCB modulator it was found the PCB layout contained

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Figure 5.12: Unpopulated Second Revision Printed Circuit Board

errors in the modulator section. As the only effective way to fix the PCB would have been

to order a third revision, a costly and time consuming endeavor, a decision was made to use

the breadboard modulator for the project. This decision was reinforced by the fact that the

PCB and breadboard modulator use identical components, save for resistor and capacitor

tolerances. Figure 5.13 shows the second order, three-state, breadboard modulator used

in the final design. Using the headers placed on the PCB to separate the various stages it

was possible to connect the breadboard modulator to the power stage inputs on the PCB.

Without these headers connecting the breadboard modulator to the power stage would have

been much more difficult.

While the modulator was being tested, a separate PCB was populated with the power

stage and filter. Functionality testing confirmed these two stages worked on the new PCB.

Figure 5.14 shows the second revision PCB with the power stage and filter sections popu-

lated, as well as the input wires from the breadboard modulator to the power stage.

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Figure 5.13: Second Order, Three State Breadboard ∆Σ Modulator

Figure 5.14: Populated Second Revision Printed Circuit Board

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Chapter 6

Final Results

The following section provides an overview of the tests performed to ensure that the final

design met the product specifications listed in Table 1.1. While this second testing procedure

did include some of the functionality tests conducted in Chapter 4, it also included perfor-

mance testing of the amplifier. The functionality testing was altered from the preliminary

testing to account for the entire amplifier being on a single PCB. After the functionality

testing, an efficiency test was conducted, as the purpose of a Class D amplifier is high effi-

ciency. Finally, the signal quality was tested to ensure that the output signal was a higher

power replica of the input signal. With the data provided by the testing, a quantitative

analysis of the amplifier could be performed, the results of which can be found at the end of

this chapter.

6.1 Functionality Test Results

The amplifier design was divided into three subsections: the modulator, the power stage, and

the filter. The functionality testing was designed to thoroughly test each individual section

and compare the actual results to the expected results. While one round of functionality

testing had already been completed, a new PCB design necessitated retesting each component

to ensure the new PCB did not contain any errors. Since the entire amplifier was on a single

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PCB instead of discrete sections extra work was taken to provide a series of test points to

isolate the three systems for testing.

6.1.1 Modulator

Similar to the first round of functionality testing, the modulator was the first component to

be tested. The criteria used to judge the test was whether or not applying a standard audio

test tone, a 1 kHz sine way, to the modulator would produce a modulated signal capable of

being amplified by the power stage. The first step to performing this test involved a simple

qualitative test: viewing a small sample of the modulator output and verifying that it was

a modulated signal at the right levels, 0 to 5 V.

It was found that there were a number of errors on the PCB version of the modulator.

Originally the modulator schematic was created as a single file and when that file was copied

into the power stage file schematic to create one comprehensive PCB, there were some traces

that were missing and went unseen. Because of time and money constraints, the modulator

was constructed on a breadboard and the result was connected to the power stage.

After confirming that the modulator was generating a modulated signal at the right levels

it could then be tested with the Power Stage to confirm the amplified signal resembled the

input signal. As discussed in Section 5 the second revision of the modulator was a second

order, three-state ∆Σ modulator, implying that were two outputs to monitor.

6.1.2 Power Stage

The power stage and filter were originally designed on a PCB because they contained several

components that could only be purchased in surface mount packages. The layout was changed

slightly for the second revision, however, as better components, like the new filter inductors,

were found. This required that functionality testing be repeated to verify that the power

stage still worked properly on the new PCB. Using two injection points it was possible to

directly apply a square wave from a function generator to the power stage. A square wave

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is unrealistic when compared to the expected modulator output, but it was a simple way to

test the power stage independently of the modulator.

As with the first power stage test, the first point to test was the driver outputs, both

low and high, to confirm that they were switching in sync with the driver input. The high

side was expected follow the input, while the low side was expected to be inverted from

the input. Once this was confirmed the next step was to test the MOSFET terminals. By

viewing the voltage drop across the MOSFET terminals it was possible to determine whether

the MOSFET was on, in the active region, or off, in the cutoff region. The MOSFETs

were expected to switch in sync with the driver outputs, if the driver output was high, the

MOSFET should have had approximately a 0 V drop across the terminals. If the driver

output was low the MOSFET should have had 40 V across the terminals.

The final power stage was fully functional. It was able to amplify square waves applied

to it.

6.1.3 Filter

The filter stage could only be tested after the power stage was working due to the balanced

nature of the filter. The same test from Section 4.1.3 was performed, though the filter

design had been slightly modified as described in Section 5.3. Again, a square wave was

passed through the power stage into the filter, using an inverter to provide the proper signal

to one driver. The frequency of the square wave was varied, from 20 Hz to 40 kHz. When

the frequency was significantly below 30 kHz, enough that several harmonics were in the

passband, a square wave was passed through the filter. When the frequency was increased

so that harmonics were blocked by the filter the output began to look more like a sine

wave. The final filter was functional. It had a fairly narrow passband and did filter out

the modulated signals back to what was expected. See Section 6.3.4 for the final frequency

response of the whole system.

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6.2 Efficiency Results

In addition to functionality testing, some performance testing was required to quantitatively

analyze the amplifier. The first performance testing conducted was the efficiency test, as a

Class D amplifier should have a very high efficiency compared to other types of amplifiers.

Efficiency is a measure of how much power going into a system passes through as useable

power to the output, or conversely, how much power is not converted into waste heat in the

system.

The efficiency of the system depends on a few different factors. The frequency of the input

signal, the output power and the switching frequency of the system can all affect efficiency.

Efficiency readings were recorded at 12 frequencies in the audio band: 20Hz, 50Hz, 100Hz,

200Hz, 500Hz, 1kHz, 2kHz, 5kHz, 10kHz, 12kHz, 15kHz and 20kHz. These were recorded at

4 different levels of output power: 40Vpk or full power, 30Vpk, 20Vpk and 10Vpk. All of these

results were recorded at 4 different switching frequencies: 1MHz, 2MHz, 5MHz and 10MHz.

All of this data is located in Appendix K.

The plot in Figure 6.1 shows the efficiencies for different signal frequencies. This data

was recorded at full output power. The plot shows that the efficiency of the final system

was above 90% at all of the clock frequencies tested while the system was at full output

power. This plot also illustrates the impact of the modulation frequency on the efficiency of

the system. The 1MHz modulation frequency was up to a few percentage points better in

terms of efficiency but because of the noise produced it was not a viable option. The sound

quality results are available in Section 6.3.

The plot in Figure 6.2 shows the efficiencies for different output levels. The efficiencies

here are much higher at high output levels. This is because ∆Σ modulation requires a lot

more switching to digitally simulate a signal at lower than full range. It is also interesting

to note that on this plot, using a switching frequency of 1MHz is actually less efficient than

the higher frequencies at an output level of 10Vpk. This is due to the excess noise that

is produced with a slower switching frequency that makes the 1MHz switching frequency

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102

103

104

90

91

92

93

94

95

96

97

98

99

100Plot for Efficiency at Full Output Power

Signal Frequency (Hz)

Effi

cien

cy (

%)

1MHz2MHz5MHz10MHz

Figure 6.1: Plot of Efficiency vs. Signal Frequency

unusable.

These plots show that the specification of greater than 90% efficiency was met. In fact,

within most of the audio band, the amplifier was able to produce efficiencies of greater than

95% which was far beyond the expectations of this project.

6.3 Sound Quality Results

Along with high efficiency the most important aspect of a Class D amplifier is the sound

quality. To determine sound quality several tests were completed, both quantitative and

qualitative. The quantitative tests looked at Total Harmonic Distortion (THD), Signal to

Noise Ratio (SNR) and Frequency Response. These three specifications can describe how

clean a signal is, or how free it is from unwanted noise. The qualitative test was a simple

listening test, playing various well known, high quality music through the amplifier, and

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5 10 15 20 25 30 35 40 4555

60

65

70

75

80

85

90

95

100Plot for Efficiency of Input Signals at f = 1kHz

Output Signal Amplitude (Vpk−pk)

Effi

cien

cy (

%)

1MHz2MHz5MHz10MHz

Figure 6.2: Plot of Efficiency vs. Output Peak Voltage

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determining how the output sounds to the human ear.

The quantitative test was a combination of testing for THD, SNR and Frequency Re-

sponse. In order to do this, a very high quality digital signal had to be recorded. This was

done by generating a signal in Matlab and using the E-MU 0202 USB sound card to apply

it to the amplifier. The signal was scaled down using a voltage divider at the output of

the amplifier and then recorded. Scaling the signal down was necessary because the sound

card could not handle a 80Vpk−pk signal. The signal was both played to the sound card and

recorded using Sonar TM. This was done because Matlab could not record at 96kbps and

24-bit, whereas Sonar could. The wavefile of the recording was saved and cropped to avoid

the transients at the beginning and end of the recording while still ensuring that it included

an integer number of periods of the signal so that a proper Fast Fourier Transform (FFT)

could be taken. Finally the wave files were opened with Matlab and the resulting data was

tested for sound quality.

6.3.1 Loopback Test

In order to determine that the test code functioned properly and that the sound card was

good enough to use to test to the specifications outlined in Section 1.1, a loopback test was

conducted. In a loopback test, the output is directly connected to the input of a sound card,

and various test sounds waves are played and recorded. Then the THD, SNR and FR tests

were conducted on the recordings. If the sound card had proved to have specifications that

were not high enough to test for the specifications of this project then it would have been

impossible to see if the amplifier met those specifcations. The plots in Figures L.1 and L.2

show the results of the loopback tests.

As these plots show, the THD for the loopback was well below 0.1% and the frequency

response was well below 0.01dB and these values are good enough to calculate a THD of 1%

and a frequency response of 3dB.

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101

102

103

104

105

1

2

3

4

5

6

7

8

9

10x 10

−3 THD vs Frequency (Loopback)

Signal Frequency (Hz)

TH

D (

%)

Figure 6.3: THD results for Loopback Test

101

102

103

104

105

−0.07

−0.06

−0.05

−0.04

−0.03

−0.02

−0.01

0Frequency Response (Loopback)

Signal Frequency (Hz)

Am

plitu

de (

dB)

with

1kH

z R

efer

ence

Figure 6.4: Frequency Response results for Loopback Test

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6.3.2 Total Harmonic Distortion

One measure of the quality of an audio signal is the Total Harmonic Distortion (THD). THD

is a relatively simple measurement, but can only be easily calculated under strict test condi-

tions. As discussed in Section 2.4.1 THD is just the ratio between the desired fundamental

frequency and all of the harmonics added together, though in practice only the first five

harmonics have a significant impact on the measurement. The easiest way to calculate THD

is to play pure audio tones because the output will be very easy to analyze. The Fast Fourier

Transform (FFT) of the output will produce a frequency domain representation of the signal

from which the fundamental and the first five harmonics can be calculated. Equation 6.1

can then be used to calculate THD:

THD =

harm21 + harm2

2 + harm23 + harm2

4 + harm25

fundamental· 100 (6.1)

The code that was used to calculate THD from the wave files is located in Appendix I.

101

102

103

104

0

0.2

0.4

0.6

0.8

1

1.2

1.4

1.6

1.8

2THD vs Frequency at 5MHz Modulation Frequency

Signal Frequency (Hz)

TH

D (

%)

Figure 6.5: THD results at 5MHz clock frequency

As shown by the plot in Figure L.9 the THD was, for the most part, below 1%. This

means that the amplifier met the specification. The only times where the result exceded the

1% barrier was at 20Hz and 20kHz. This was because the test equipment could not handle

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extremely low frequencies and the signal was probably attenuated more than expected at

20kHz. This is a reasonable specification for the product because there is not a lot of sound

at those frequencies.

6.3.3 Signal To Noise Ratio

Another important measure of audio quality is the Signal to Noise Ratio (SNR). Section 2.4.1

describes SNR in detail. SNR is important for high power devices because a device with a

low SNR will create an audible “hiss” in the speakers. That hissing is actually the noise

floor of the signal, meaning that is the quietest the signal can be. The equation for SNR is

given in Equation 2.3. The code that was used to calculate SNR from the recorded wave

files is located in Appendix I.

101

102

103

104

105

89

89.5

90

90.5

91

91.5

92

92.5SNR vs Frequency at 5MHz Modulation Frequency

Signal Frequency (Hz)

SN

R (

dB)

Figure 6.6: Plot of SNR vs. Frequency

The SNR was calculated by first recording a the output of the amplifier at each of the

frequencies recorded for each of the other sound quality measurements. The signal power was

derived from this recording. Then the output of the amplifier with no input was recorded.

This allowed for the recording of the noise floor without a signal or harmonics to interfere.

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The total power was summed over the audio band to develop the total noise power. The

SNR was then calculated using Equation 2.3. Figure L.10 shows a plot of the SNR versus

frequency.

These results indicate that the amplifier met the SNR specification, in that it was greater

than 90dB, for most of the frequencies in the audio band. At the upper end of the frequency

spectrum, around 20kHz, the SNR falls just below 90dB, but it is at a frequency that is

difficult to hear and it only falls to 89dB. This is probably a result of the beginning of the

cutoff of the filter. Further SNR plots are available in Appendix L.

6.3.4 Frequency Response

The final measure of audio quality is the frequency response. Frequency response is different

from THD and SNR in that it is not measuring noise, but determining how flat the passband

of the amplifier is. Ideally the amplifier will have a perfectly flat passband from 20 Hz to 20

kHz, though practical limitations may result in slight deviations. To the human ear these

deviations will be manifested by different audio levels for different frequencies. As long as

the deviations are within +1 dB a listener will generally not notice. Equation 4.5 can be

used to calculate the frequency response.

The plot in Figure L.11 shows the frequency response. In this plot the gain at 1kHz is

the 0dB reference and all other gains are the amount of dB outside of that reference. Up

until 20kHz the response is definitely within 3dB of the 1kHz reference. However, at 20kHz

the specification is not met. This is probably due to the response of the filter because of

how inaccurate it is. This is okay, however, because there is not a lot of audio information

at that high of a frequency since most people cannot hear that. Another interesting note

about this result is that at 1MHz the frequency response goes higher at 20kHz and all the

other clock frequencies result in the frequency response decreasing. This is another example

of how the system developed does not work with a switching frequency of 1MHz.

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101

102

103

104

105

−3

−2.5

−2

−1.5

−1

−0.5

0Frequency Response at 5MHz Modulation Frequency

Signal Frequency (Hz)

Am

plitu

de (

dB)

with

1kH

z R

efer

ence

Figure 6.7: Plot of Efficiency vs. Output Peak Voltage

6.3.5 Listening Test

The listening test is a highly subjective test dependent upon the tester’s musical ability. The

purpose of this test is not to quantitatively identify problems, but instead to qualitatively

pass or fail the amplifier design. While there is no specific song used in this test, the tester

was encouraged to pick a song they knew well, one that they felt would be easy to find

unwanted noise. This means that a “CD Quality” recording is needed, as poor quality audio

recording will contain noticeable noise that may confuse the tester.

While playing the song through the amplifier, the tester must be sure to listen careful

for any sort of static or noise. If noise is detected a note should be made of the approximate

time in the audio track. If after several plays the same areas are determined to be noisy

an FFT should be taken of the audio recording as well as the amplifier output at the same

time. This will allow for a comparison to be made, and will help determine if the noise is

inherent to the audio recording or being caused by the amplifier.

The amplifier was able to play music from a computer that “sounded good” to multiple

testers. This qualitative measurement was important because the numbers and readings

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mean nothing unless the amplifier actually functions correctly.

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Chapter 7

Conclusion

The ultimate goal of this project was to design and build a fully functional Class D audio

amplifier. Original project specifications included greater than 90% efficiency and less than

1% Total Harmonic Distortion (THD). Additonal project goals were 80 Watt Output Power

and a Signal to Noise Ratio (SNR) of 90 dB. A test plan was also developed in order to

determine if these goals and specifications were met and to determine if this project was

successful.

The first step in accomplishing this project was to develop an understanding of how

Class D amplifiers function. This was accomplished by researching past projects as well as

commercial products. Once an understanding of Class D amplifiers was obtained several

Matlab simulations were created. These simulations allowed for various methods and

components to be tested, ultimately saving valuable time and money in the final design.

After completing simulations the project shifted gears to begin developing working pro-

totypes. The first stage completed was the power stage. The power stage was developed

directly to a printed circuit board (PCB) because the MOSFETs used only came in surface

mount packages, in order to maintain extremely high efficiencies. This did result in some

complications as design flaws were more difficult to work around on a PCB as compared to

a breadboard. The power stage PCB was ultimately a success, however, proving that the

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project design and component choices worked. The first filter was developed alongside the

power stage. This helped to minimize losses in output power by keeping power traces very

short on the PCB, instead of requiring cabling to a separate board for the filter. The first

power stage PCB was able to output an 80Vpk−pk signal, resulting in 80W power output to

an 8Ω load.

While the power stage was being developed, a first order ∆Σ modulator was developed

on a breadboard. This first order modulator was capable of modulating a signal, though it

did not produce a high enough SNR to meet the project goal. The first order modulator

proved extremely useful, however, for testing the power stage and filter to ensure that they

could properly amplify a modulated signal. Using this first full system prototype the design

of the amplifier was tested by performing various functionality tests. A full performance

test was not completed, as simulations showed that this design would not meet the original

project specifications.

Using test results from the prototype system and additional research a second order ∆Σ

modulator was developed. A higher order modulator allowed for a higher SNR due to more

control over where noise is generated. The switching frequency of the modulator was also

increased, from 1 MHz to 5 MHz. This helped to push modulation noise well above the

audio band, which was also instrumental in increasing the SNR of the amplifier without

significantly reducing efficiency. While the second order modulator was developed work was

done to slightly alter the filter. The filter was changed to a higher cutoff frequency, 30 kHz

instead of 25 kHz, in an effort to increase efficiency and ensure the entire audio band is

properly passed through the amplifier. The 30 kHz cutoff frequency was also decided upon

by the inductor values found. The particular inductor used for the filter was both inexpensive

and had an extremely low equivalent series resistance which was crucial in helping to minimize

power loss in the system.

After the second order ∆Σ modulator was designed a second revision of the PCB was

developed. In addition to having the modulator, power stage, and filter on one board, the

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second revision PCB was significantly smaller than the first revision, which only had the

power stage and filter. The smaller size was ideal for a production environment, as a smaller

footprint may result in lower production costs. Unfortunately, the modulator on the second

revision of the PCB had several issues which could not be resolved without ordering a new

PCB, a costly and time consuming process. Due to the costs involved with ordering a new

PCB, the decision was made to keep the second order modulator on a breadboard.

Finally, after confirming that the second revision system worked a series of performance

testing was done to ensure the amplifier design met the original specifications. The perfor-

mance testing was done using a high end computer sound card and Matlab to generate test

tones and record and analyze the system output. This setup allowed for semi-automated

testing, by developing a Matlab script to cycle through the frequencies of interest. The

efficiency testing had to be performed by hand as measuring power in and power out required

the use of an ammeter and two voltmeters, in addition to input test tones.

The result was that the amplifier met most of the specifications. The frequency response

was well below 3dB for most of the audio band, THD was below 1%, SNR was around 92dB

for most of the audio band and most importantly the efficiency was above 90%. In fact, the

efficiency reached over 95% for almost all frequencies at full output power.

This project was successful. While there were several issues in the development of the

final product, the end result was a working Class D audio amplifier that met the original

project specifications. While the final design was not implemented completely on a single

PCB, the completed layout shows how small a final production design of this amplifier could

be. While the accomplishments of this project are significant, there are several areas of

future research that were beyond the scope of the project.

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Chapter 8

Future Work & Recommendations

While this project was successful in designing and implementing a fully functional Class D

audio amplifier there are many additional areas that can be explored to complement the

completed Class D audio amplifier. The focus of this project was to develop an amplifier to

drive an 8Ω load. However, a working amplifier is a component that can be used in many

different products, from guitar amplifiers to home theater receivers. This section will discuss

several of the ideas for future work concerning Class D audio amplifiers.

8.1 High Efficiency Power Supply

While an amplifier can be thought of as simply a transistor that amplifies an input signal,

a finished product is much more than that. While the major accomplishment of this MQP

was a completed Class D audio amplifier, it was tied to the lab bench due to the need for

a power supply. To be considered a finished commercial product an amplifier must have its

own dedicated power supply, ideally one that can be plugged into a standard wall outlet

or a high power battery. The power supply would have to provide several different voltage

rails, ranging from 5 Volts to 40 Volts, for different parts of the modulator and power stage.

Since the power supply would be for a Class D audio amplifier it would need to be an

extremely high-efficiency power supply. Otherwise the efficiency of the entire system could

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drop to unacceptable levels. Any work undertaken to develop such a power supply should also

consider the power requirements of running multiple amplifiers in parallel. Many professional

quality amplifiers offer 2 or 4 channels per amplifier unit, usually for stereo or surround sound

systems. See Section 8.4 for further recommendations regarding multichannel amplifier units.

8.2 PCB Modulator with Full System Feedback

While this project did develop a fully working system, the final product was still a proto-

type design. One reason for this was that the modulator was never successfully assembled

on a PCB due to complications with routing feedback lines, which are necessary for the

modulator to run properly. Moving to a PCB may help reduce unwanted noise and increase

the performance of the modulator. When moving to a PCB, full system feedback could be

implemented. If the output of the amplifier were scaled and subtracted from the input, any

noise or error introduced by the system could be compensated for, and the overall sound

quality of the system would be improved. Full system feedback was not considered in this

project because introducing another level of feedback to the modulator has the potential

to destabilize the system. In addition, full system feedback could introduce more noise due

to long cabling when not implemented directly on a PCB. A final complication that would

need to be solved is the problem of delay. Within the modulator, the feedback delay is small

enough that little to no effect is noticed, and the modulator functions within the specifica-

tions. With full system feedback, however, the delay would be increased significantly and

could cause the feedback to decrease the sound quality rather than improve it.

8.3 Digital Input

Another area untouched by this project was the realm of digital audio signals. Currently,

most live audio is generated, mixed, and amplified in the analog domain. However, many

of the newer mixing consoles are digital. While these digital boards maintain analog inputs

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and outputs, this is due to the analog nature of the devices they communicate with. Digital

signals contain many advantages, from reduced Electromagnetic Interference (EMI) noise to

being able to send multiple signals on one wire, or even wirelessly. A digital signal would not

need to be modulated, but a parallel stage would be required to convert the digital signal

so that it could be properly recognized and amplified by the power stage. Depending on the

type of conversion used, there could be much less noise than would be generated by even a

second order ∆Σ modulator.

In addition to the professional audio market, many home theater applications offer digital

chains straight from the source material to the amplifier. The amplifier developed as a part

of an MQP would be an ideal candidate for developing a high power, high efficiency home

theater receiver. More information regarding digital audio is available in Appendix M.

8.4 Multichannel Systems

As previously discussed, the amplifier developed in this project is ideal for creating multi-

channel systems. This would be applicable to both professional and home audio. Professional

audio amplifiers generally have either two or four channels per amplifier unit. This is be-

cause most sound systems are setup in symmetrical pairs, for left and right audio channels.

However, many professional speakers contain multiple drivers, each powered by a single am-

plifier. Generally these systems use between two and four individually powered drivers per

speaker, essentially placing multiple speakers in one cabinet. A quad channel amplifier unit,

using the amplifier developed by this MQP, would allow for a small, but extremely power-

ful package to drive professional sound systems. Such a project would require an intensive

signals portion, to provide proper crossovers for each channel, as well as to ensure that the

gain of each channel is identical.

Developing a multichannel amplifier for home theater systems would have similar, but

different issues. First, a replacement for the modulator would need to be designed to decode

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the home theater audio signals, which are now usually in a digital format. Controls would

need to be designed to adjust volume and equalize each channel independently, as well as

all of the channels together. Research into current home theater systems would be needed

to determine other features.

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Bibliography

[AES05] Aes standard for digital audio engineering - high-resolution multi- channel audio

interconnection (hrmai). Technical report, 2005.

[AVM08] Aviom16/o-y1, a-net card for yamaha. Technical report, 2008.

[Ber03] Mark Berkhout. An integrated 200W Class D audio amplifier. IEEE Journal of

Solid-State Circuits, 38(7):1198–1206, July 2003.

[Dal97] Enrico Dallago. Advances in high-frequency power conversion by delta-sigma mod-

ulation. IEEE Transactions on Circuits and Systems, 44(8):712–721, August 1997.

[HA05] Jun Honda and Jonathan Adams. Class D audio amplifier basics. Application

Note AN-1071, International Rectifier, 2005.

[IRF07] IR introduces integrated and protected Class D audio chipset for small, high per-

formance amplifiers. 2007.

[Lac91] Kerry Lacanette. A basic introduction to filters - active, passive and switched-

capacitor. Technical report, Swarthmore, April 1991.

[Max06] Class D amplifiers: Fundamentals of operation and recent developments. Appli-

cation Note AN-3977, Maxim, 2006.

[McD01] Duncan McDonald. Class D audio-power amplifiers: Interactive simulations assess

device and filter performnance. Technical report, January 2001.

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[MDS08] Xl8 specifications. Technical report, 2008.

[Qui93] Patrick Quilter. Amplifier anatomy - part 1. Technical report, February 1993.

[SNY08] Hypermac protocol. Technical report, 2008.

[ST05] Richard Schreier and Gabor C. Temes. Understanding Delta-Sigma Data Convert-

ers. Wiley- IEEE Press, 2005.

[TI:99] Design considerations for Class D audio power amplifiers. Technical report, August

1999.

[YMH07] Ls-9 specifications. Technical report, 2007.

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Appendix A

First Order ∆Σ Modulation: Matlab

Simulation Code

The following is the code that was used to simulate first order delta sigma modulation prior

to hardware construction.

% This function simulates first order delta sigma modulation without feedback.

% Its intended application is the Class D Audio Amplifier MQP, to be used with

% input signals in the audio band to assess noise and modulation techniques.

function output = dssim2(sigfreq, modfreq, simlength,C,R1,R2,Vqout,Vthres)

% Set sampling frequency

fs = modfreq*100;

% Create a basic sine wave

t = linspace(0,simlength-1/fs,fs*simlength);

f = sin(sigfreq*2*pi*t);

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tqon=1/modfreq;

% Modulate!

bias = -max(f);

f=f+bias;

output = zeros(1,length(t));

dlatchstate = 0;

intvalue = Vthres-eps;

check = 0;

for i = 1:length(t)

intvalue = intvalue - (1/(R1*C*fs))*f(i) - dlatchstate*(1/(R2*C*fs))*Vqout;

if mod(i,100)==0

if intvalue > Vthres

dlatchstate=1;

else

check = check + dlatchstate;

dlatchstate=0;

end

end

output(i)=1-dlatchstate;

end

check

%Plot fft

figure;

semilogx(linspace(0,fs,length(output)),20*log10(abs(fft(output))));

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xlabel(’Frequency (Hz)’);

ylabel(’Amplitude (dB)’);

title(’Delta Sigma Modulation’);

sfft=abs(fft(output));

snrreg = sfft(11)/sum(sfft(15:floor(length(sfft)/2)));

dBsnr = 20*log10(snrreg);

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Appendix B

Matlab Script to Find ‘a’ Coefficients

The following script was used to determine a1, a2, and a3, and was taken from Schreier’s

Understanding Delta-Sigma Data Converters [ST05].

%Desired NTF and its impulse response

NTF = zpk([1,1],[1,1]/3,1,1);

n_imp = 10;

y_desired = impL1(NTF,n_imp)’);

% State-space description of CT loop filter

% as a 3-input, 1-output system

Ac = [0 0; 1 0 ];

Bc = [-1 0 0; 0 -1 0];

Cc = [0 1];

Dc = [0 0 -1];

td = 0.5;

sys_c = ss(Ac,Bc,Cc,Dc);

set(sys_c,’InputDelay’,td*[1 1 1]);

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%discrete-time equivalend and associated impulse repsonse

sy_d = c2d(sys_c,1)

yy = squeeze(impulse(sys_d,n_imp))’;

%Solve for coefficients s.t. a*yy = y_desired

a = y_desired/yy;

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Appendix C

First Order ∆Σ Modulation: Matlab

Simulation Code

% This function simulates second order delta sigma modulation. Its

% intended application is the Class D Audio Amplifier MQP, to be used with

% input signals in the audio band to assess noise and modulation techniques.

function qoutput = secondorderdsm(sigfreq, modfreq, simlength)

% Set output pulsewidth and the reset voltage threshold for the d-latch and

% integrator

fs = modfreq*100;

%Create a basic sine wave

t = linspace(0,simlength-1/fs,fs*simlength);

f = sin(sigfreq*2*pi*t);

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% insert test values

tqon=1/modfreq;

a1=4/9;

a2=1+3/9;

a3=11/18;

b1=1/3;

c1=modfreq;

c2=modfreq;

% Modulate!

qoutput = zeros(1,length(t));

c1output = zeros(1,length(t));

c2output = zeros(1,length(t));

T=1/fs;

qstate = 0;

c1value = 0;

c2value = 0;

check = 0;

for i = 1:length(t)

c1value = c1value + (1/(fs))*(b1*f(i) - qstate*a1);

c2value = c2value + (1/(fs))*(c1*c1value - qstate*a2);

qin = c2value*c2 - a3*qstate;

if mod(i,100)==0

if qin > 0.5

qstate = 1;

elseif qin < -0.5

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qstate = -1;

else

qstate = 0;

end

end

qoutput(i)=qstate;

c1output(i)=c1*c1value;

c2output(i)=c2*c2value;

end

plot(t,5*qoutput,’b’,t,f,’r’);

semilogx(linspace(0,fs,length(qoutput)),20*log10(abs(fft(qoutput))),’b’);

xlabel(’Frequency (Hz)’);

ylabel(’Amplitude (dB)’);

title(’Delta Sigma Modulation (System Model)’);

max(20*log10(abs(fft(qoutput))))

end

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Appendix D

MOSFET Equation Derivations

This appendix outlines the derivations for the equations in Section 3.2. These calculations

were provided by Professor John McNeill.

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Appendix E

MOSFET Losses: Matlab Simulation

Code

This appendix contains the code used to determine the loss curves for a variety of MOSFETs.

figure;

%Range of Switching Frequencies

fSw = 40000:10:5000000;

vDrive = 20;

%Filter Values

rC = 0.01;

c = 36*10^-6;

rL = 0.01;

l = 0.56*10^-6;

%Other Values

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rLoad = 4;

vPk = 40;

iOut = 5;

%MOSFET Values

hold all;

%IRF3805

rDS = 3.3*10^-3;

tOn = 150*10^-9;

tOff = 93*10^-9;

cGS = 7960*10^-12;

pInductor = (vPk.^2).*rL./(192.*(l.^2).*(fSw.^2));

pCapacitor = vPk.^2./(192.*(rLoad.^2).*rC.*(c.^2).*(fSw.^2));

pRDS = ones(size(fSw)).*rDS.*(iOut.^2);

pSwitch = (tOn + tOff).*(vPk./rLoad).*fSw;

pCgs = fSw.*cGS.*vDrive;

pTotal = pInductor + pCapacitor + pRDS + pSwitch + pCgs;

loglog(fSw, pTotal);

%IRF1010

rDS = 8.5*10^-3;

tOn = 90*10^-9;

tOff = 54*10^-9;

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cGS = 2810*10^-12;

pInductor = (vPk.^2).*rL./(192.*(l.^2).*(fSw.^2));

pCapacitor = vPk.^2./(192.*(rLoad.^2).*rC.*(c.^2).*(fSw.^2));

pRDS = ones(size(fSw)).*rDS.*(iOut.^2);

pSwitch = (tOn + tOff).*(vPk./rLoad).*fSw;

pCgs = fSw.*cGS.*vDrive;

pTotal = pInductor + pCapacitor + pRDS + pSwitch + pCgs;

loglog(fSw, pTotal);

%IRF3808

rDS = 7*10^-3;

tOn = 140*10^-9;

tOff = 120*10^-9;

cGS = 5310*10^-12;

pInductor = (vPk.^2).*rL./(192.*(l.^2).*(fSw.^2));

pCapacitor = vPk.^2./(192.*(rLoad.^2).*rC.*(c.^2).*(fSw.^2));

pRDS = ones(size(fSw)).*rDS.*(iOut.^2);

pSwitch = (tOn + tOff).*(vPk./rLoad).*fSw;

pCgs = fSw.*cGS.*vDrive;

pTotal = pInductor + pCapacitor + pRDS + pSwitch + pCgs;

loglog(fSw, pTotal);

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%IRF3205

rDS = 6.5*10^-3;

tOn = 95*10^-9;

tOff = 67*10^-9;

cGS = 3450*10^-12;

pInductor = (vPk.^2).*rL./(192.*(l.^2).*(fSw.^2));

pCapacitor = vPk.^2./(192.*(rLoad.^2).*rC.*(c.^2).*(fSw.^2));

pRDS = ones(size(fSw)).*rDS.*(iOut.^2);

pSwitch = (tOn + tOff).*(vPk./rLoad).*fSw;

pCgs = fSw.*cGS.*vDrive;

pTotal = pInductor + pCapacitor + pRDS + pSwitch + pCgs;

loglog(fSw, pTotal);

%IRF1405

rDS = 4.9*10^-3;

tOn = 110*10^-9;

tOff = 82*10^-9;

cGS = 4780*10^-12;

pInductor = (vPk.^2).*rL./(192.*(l.^2).*(fSw.^2));

pCapacitor = vPk.^2./(192.*(rLoad.^2).*rC.*(c.^2).*(fSw.^2));

pRDS = ones(size(fSw)).*rDS.*(iOut.^2);

pSwitch = (tOn + tOff).*(vPk./rLoad).*fSw;

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pCgs = fSw.*cGS.*vDrive;

pTotal = pInductor + pCapacitor + pRDS + pSwitch + pCgs;

loglog(fSw, pTotal);

%IRF6645

rDS = 28*10^-3;

tOn = 5*10^-9;

tOff = 5.1*10^-9;

cGS = 890*10^-12;

pInductor = (vPk.^2).*rL./(192.*(l.^2).*(fSw.^2));

pCapacitor = vPk.^2./(192.*(rLoad.^2).*rC.*(c.^2).*(fSw.^2));

pRDS = ones(size(fSw)).*rDS.*(iOut.^2);

pSwitch = (tOn + tOff).*(vPk./rLoad).*fSw;

pCgs = fSw.*cGS.*vDrive;

pTotal = pInductor + pCapacitor + pRDS + pSwitch + pCgs;

loglog(fSw, pTotal);

%IRF6665

rDS = 53*10^-3;

tOn = 2.8*10^-9;

tOff = 4.3*10^-9;

cGS = 530*10^-12;

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pInductor = (vPk.^2).*rL./(192.*(l.^2).*(fSw.^2));

pCapacitor = vPk.^2./(192.*(rLoad.^2).*rC.*(c.^2).*(fSw.^2));

pRDS = ones(size(fSw)).*rDS.*(iOut.^2);

pSwitch = (tOn + tOff).*(vPk./rLoad).*fSw;

pCgs = fSw.*cGS.*vDrive;

pTotal = pInductor + pCapacitor + pRDS + pSwitch + pCgs;

loglog(fSw, pTotal);

hold off;

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Appendix F

MOSFET Data Sheet

This appendix contains the data sheet for the IRF6645, the MOSFET used in the power

stage.

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Appendix G

Preliminary Schematic

The schematic shown in Figure G.1 represents a preliminary system design.

Figure G.1: A preliminary schematic

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Appendix H

Final Schematics

The following appendix gives the schematics for the preliminary design and the final design.

Figure H.1: Preliminary Schematic of the Power and Filter Stages

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Figure H.2: Final Schematic - Modulator

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Figure H.3: Final Schematic - Power Stage and Filter

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Appendix I

Final Matlab Test Code

The following appendix gives the Matlab code that was used to test the amplifier.

I.1 Efficiency

getValues.m

numFreqz = 12;

numAmps = 4;

numSwitch = 4;

amplitudes = [40,30,20,10];

freqz = [20,50,100,200,500,1000,2000,5000,10000,12000,15000,20000];

switches = [1,2,5,10];

efficiency = zeros(numSwitch,numAmps,numFreqz);

tempArr = zeros(numFreqz);

for k = 1:numSwitch

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if k==1

filename = ’M:\MQP\final Efficiency Results\Efficiency - 1MHz’;

end

if k==2

filename = ’M:\MQP\final Efficiency Results\Efficiency - 2MHz’;

end

if k==3

filename = ’M:\MQP\final Efficiency Results\Efficiency - 5MHz’;

end

if k==4

filename = ’M:\MQP\final Efficiency Results\Efficiency - 10MHz’;

end

for i = 1:numAmps

tempArr = xlsread(filename,i,’m2:m13’);

for j=1:numFreqz

efficiency(k,i,j) = tempArr(j)*100;

end

end

end

plotAmplitudeX.m

close all;

amplitudes = [40,30,20,10];

ampArr = zeros(1,numAmps);

figure;

hold all;

for i=1:numSwitch

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for j=1:numAmps

ampArr(j) = efficiency(i,j,6); % take the 1kHz values

end

plot(amplitudes, ampArr);

end

title(’Plot for Efficiency of Input Signals at f = 1kHz’);

xlabel(’Output Signal Amplitude (Vpk-pk)’);

ylabel(’Efficiency (%)’);

legend(’1MHz’,’2MHz’,’5MHz’,’10MHz’);

axis([5, 45, 55, 100]);

hold off;

plotFreqX.m

close all;

freqArr = zeros(1,numFreqz);

figure;

hold all;

for i=1:numSwitch

for j=1:numFreqz

freqArr(j) = efficiency(i,1,j); % take the 1kHz values

end

semilogx(freqz, freqArr);

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end

title(’Plot for Efficiency at Full Output Power’);

xlabel(’Signal Frequency (Hz)’);

ylabel(’Efficiency (%)’);

legend(’1MHz’,’2MHz’,’5MHz’,’10MHz’);

axis([20, 20e3, 90, 100])

hold off;

I.2 THD

THD.m

function THD = THD(signal, f, fs)

numHarm = 5;

harm = zeros(1, numHarm);

N=length(signal);

n=round(floor(N/fs*f)*fs/f); % # samples for whole number of periods

signal=signal(1:n);

SIG = abs(fft(signal));

SIG = SIG/max(SIG); % normalize the fft

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[fund fundIndex] = max(SIG); % find the fundamental frequency

f = linspace(0,fs,length(signal));

fundFreq = f(fundIndex);

for i=1:numHarm % each iteration of the loop finds a new harmonic

for j = 1:length(f) % loop through to find the harmonic

if f(j) >= (i + 1)*fundFreq

harmFreq = f(j); % output the frequency of the harmonic

harm(i) = max(SIG(j-50:j+50));

break;

end

end

end

% output all the values

SIG(fundIndex)

for i=1:numHarm

harm(i)

end

% calculate the distortion

sumDist = 0;

for i=1:numHarm

sumDist = sumDist + harm(i) * harm(i);

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end

% calculate the THD

THD = sqrt(sumDist) * 100;

I.3 SNR

SNR.m

function snr = SNR(unk, noise)

%unk is the output signal, noise is the recorded "nothing" through the system

SIG = abs(fft(unk));

sigpwr = max(SIG)^2;

noisepwr = sum(noise.^2);

snr = 10*log10(sigpwr/noisepwr);

\sectionFrequency Response

\titlelineskip

\textitplotFreqResponse.m

\beginverbatim

inputRMS = input/(2*sqrt(2));

gain = zeros(1,numFreqz);

figure;

hold all;

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for i=1:numSwitch

for j=1:numFreqz

gain(j) = output(i,j)/inputRMS(i);

end

reference = gain(6);

gain = gain/reference;

semilogx(freqz,20*10*log(gain));

end

title(’Frequency Response at Full power’);

xlabel(’Signal Frequency (Hz)’);

ylabel(’Gain (dB)’);

legend(’1MHz’,’2MHz’,’5MHz’,’10MHz’);

hold off;

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Appendix J

Preliminary Efficiency Test Results

The following efficiency data was taken using a 1MHz, first order, two-level ∆Σ modulator.

Using an input sine wave with a Vpk−pk of 1.54V:Input Freq. (Hz) Vin (VDC ) Iin (ADC ) Vout (VRMS) Resistance (Ω) Pin (W) Pout (W) Efficiency (%)

20 39.86 0.2 6.65 8.05 7.972 5.493478261 68.90966208

50 39.86 0.22 6.65 8.05 8.7692 5.493478261 62.64514734

100 39.86 0.22 6.65 8.05 8.7692 5.493478261 62.64514734

200 39.86 0.22 6.65 8.05 8.7692 5.493478261 62.64514734

500 39.87 0.22 6.65 8.05 8.7714 5.493478261 62.62943499

1000 39.87 0.22 6.63 8.05 8.7714 5.460484472 62.25328308

2000 39.87 0.219 6.59 8.05 8.73153 5.394795031 61.78522013

5000 39.86 0.215 6.41 8.05 8.5699 5.104111801 59.5585923

10000 39.86 0.202 5.98 8.05 8.05172 4.442285714 55.17188519

12000 39.87 0.195 5.8 8.05 7.77465 4.178881988 53.75009792

15000 39.87 0.187 5.5 8.05 7.45569 3.757763975 50.40129049

20000 39.87 0.17 4.98 8.05 6.7779 3.080795031 45.45353326

Using an input sine wave with a Vpk−pk of 2.2V:Input Freq. (Hz) Vin (VDC ) Iin (ADC ) Vout (VRMS) Resistance (Ω) Pin (W) Pout (W) Efficiency (%)

20 39.83 0.3 8.89 8.05 11.949 9.817652174 82.1629607

50 39.84 0.332 8.9 8.05 13.22688 9.839751553 74.39208304

100 39.85 0.332 8.9 8.05 13.2302 9.839751553 74.37341501

200 39.85 0.332 8.9 8.05 13.2302 9.839751553 74.37341501

500 39.84 0.331 8.89 8.05 13.18704 9.817652174 74.44924846

1000 39.84 0.331 8.86 8.05 13.18704 9.751503106 73.94762665

2000 39.84 0.328 8.8 8.05 13.06752 9.619875776 73.61669067

5000 39.84 0.32 8.53 8.05 12.7488 9.038621118 70.89781876

10000 39.86 0.296 7.92 8.05 11.79856 7.792099379 66.04279996

12000 39.86 0.285 7.65 8.05 11.3601 7.269875776 63.99482202

15000 39.86 0.267 7.23 8.05 10.64262 6.49352795 61.01437381

20000 39.87 0.239 6.5 8.05 9.52893 5.248447205 55.07908238

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Using an input sine wave with a Vpk−pk of 2.8V:Input Freq. (Hz) Vin (VDC ) Iin (ADC ) Vout (VRMS) Resistance (Ω) Pin (W) Pout (W) Efficiency (%)

20 39.8 0.5 11.16 8.05 19.9 15.47150311 77.74624676

50 39.81 0.479 11.17 8.05 19.06899 15.49924224 81.2798278

100 39.78 0.479 11.17 8.05 19.05462 15.49924224 81.34112481

200 39.93 0.486 11.22 8.05 19.40598 15.63831056 80.58500812

500 39.79 0.478 11.15 8.05 19.01962 15.44378882 81.19925014

1000 39.79 0.478 11.1 8.05 19.01962 15.30559006 80.47263858

2000 39.79 0.474 11 8.05 18.86046 15.0310559 79.69612565

5000 39.79 0.458 10.61 8.05 18.22382 13.9841118 76.73534858

10000 39.8 0.418 9.8 8.05 16.6364 11.93043478 71.71283921

12000 39.8 0.4 9.45 8.05 15.92 11.09347826 69.68265239

15000 39.81 0.369 8.88 8.05 14.68989 9.79557764 66.68244377

20000 39.82 0.321 7.93 8.05 12.78222 7.81178882 61.114492

Using an input sine wave with a Vpk−pk of 3.2V:Input Freq. (Hz) Vin (VDC ) Iin (ADC ) Vout (VRMS) Resistance (Ω) Pin (W) Pout (W) Efficiency (%)

20 39.8 0.7 13.45 8.05 27.86 22.47236025 80.66173815

50 39.77 0.661 13.46 8.05 26.28797 22.50578882 85.61250192

100 39.78 0.661 13.46 8.05 26.29458 22.50578882 85.59098042

200 39.77 0.661 13.45 8.05 26.28797 22.47236025 85.48533892

500 39.77 0.66 13.44 8.05 26.2482 22.43895652 85.48760114

1000 39.76 0.66 13.39 8.05 26.2416 22.27231056 84.87405707

2000 39.77 0.654 13.25 8.05 26.00958 21.80900621 83.84989766

5000 39.77 0.628 12.73 8.05 24.97556 20.13079503 80.60197662

10000 39.79 0.564 11.65 8.05 22.44156 16.85993789 75.12819023

12000 39.79 0.538 11.22 8.05 21.40702 15.63831056 73.0522537

15000 39.73 0.496 10.5 8.05 19.70608 13.69565217 69.49962739

20000 39.8 0.416 9.31 8.05 16.5568 10.76721739 65.03199526

Using an input sine wave with a Vpk−pk of 3.8V:Input Freq. (Hz) Vin (VDC ) Iin (ADC ) Vout (VRMS) Resistance (Ω) Pin (W) Pout (W) Efficiency (%)

20 39.73 0.9 15.78 8.05 35.757 30.9327205 86.50815364

50 39.73 0.879 15.79 8.05 34.92267 30.97193789 88.68719914

100 39.73 0.879 15.78 8.05 34.92267 30.9327205 88.57490134

200 39.74 0.878 15.78 8.05 34.89172 30.9327205 88.65346993

500 39.74 0.876 15.73 8.05 34.81224 30.73700621 88.29367548

1000 39.74 0.873 15.65 8.05 34.69302 30.42515528 87.6982035

2000 39.77 0.864 15.48 8.05 34.36128 29.76775155 86.63167249

5000 39.79 0.823 14.82 8.05 32.74717 27.28352795 83.31568178

10000 39.84 0.728 13.45 8.05 29.00352 22.47236025 77.48149276

12000 39.84 0.686 12.87 8.05 27.33024 20.57601242 75.28661447

15000 39.85 0.616 11.97 8.05 24.5476 17.79886957 72.50757534

20000 39.85 0.53 10.65 8.05 21.1205 14.08975155 66.71125945

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Using an input sine wave with a Vpk−pk of 4V:Input Freq. (Hz) Vin (VDC ) Iin (ADC ) Vout (VRMS) Resistance (Ω) Pin (W) Pout (W) Efficiency (%)

20 39.8 1.2 18.16 8.05 47.76 40.96715528 85.77712579

50 39.8 1.16 18.18 8.05 46.168 41.05744099 88.93051679

100 39.8 1.156 18.17 8.05 46.0088 41.01228571 89.14008997

200 39.8 1.156 18.17 8.05 46.0088 41.01228571 89.14008997

500 39.82 1.153 18.12 8.05 45.91246 40.78688199 88.8361939

1000 39.82 1.149 18.03 8.05 45.75318 40.3827205 88.26210658

2000 39.83 1.136 17.8 8.05 45.24688 39.35900621 86.98722699

5000 39.84 1.078 16.97 8.05 42.94752 35.77402484 83.29706778

10000 39.8 0.909 15.26 8.05 36.1782 28.92765217 79.95879334

12000 39.81 0.854 14.6 8.05 33.99774 26.47950311 77.88606862

15000 39.83 0.772 13.57 8.05 30.74876 22.87514286 74.39370842

20000 39.84 0.68 12.02 8.05 27.0912 17.94787578 66.24983676

Using an input sine wave with a Vpk−pk of 4.8V:Input Freq. (Hz) Vin (VDC ) Iin (ADC ) Vout (VRMS) Resistance (Ω) Pin (W) Pout (W) Efficiency (%)

20 39.76 1.1 18.09 8.05 43.736 40.65193789 92.94845868

50 39.75 1.13 18.09 8.05 44.9175 40.65193789 90.50356295

100 39.73 1.13 18.09 8.05 44.8949 40.65193789 90.54912226

200 39.72 1.13 18.08 8.05 44.8836 40.60700621 90.471812

500 39.73 1.13 18.04 8.05 44.8949 40.42752795 90.04926606

1000 39.72 1.124 17.94 8.05 44.64528 39.98057143 89.55161985

2000 39.73 1.11 17.73 8.05 44.1003 39.05004969 88.54826314

5000 39.73 1.049 16.88 8.05 41.67677 35.39557764 84.9287928

10000 39.74 0.918 15.24 8.05 36.48132 28.85187578 79.08671007

12000 39.78 0.856 14.54 8.05 34.05168 26.26231056 77.12486009

15000 39.79 0.776 13.5 8.05 30.87704 22.63975155 73.32228592

20000 39.82 0.665 12.08 8.05 26.4803 18.12750311 68.45656245

Using an input sine wave with a Vpk−pk of 5.28V:Input Freq. (Hz) Vin (VDC ) Iin (ADC ) Vout (VRMS) Resistance (Ω) Pin (W) Pout (W) Efficiency (%)

20 39.76 1.7 22.83 8.05 67.592 64.7464472 95.79010416

50 39.78 1.74 22.84 8.05 69.2172 64.80318012 93.62294361

100 39.78 1.739 22.84 8.05 69.17742 64.80318012 93.67678084

200 39.78 1.739 22.82 8.05 69.17742 64.68973913 93.51279526

500 39.78 1.737 22.78 8.05 69.09786 64.46315528 93.29254955

1000 39.77 1.73 22.67 8.05 68.8021 63.84209938 92.79091682

2000 39.77 1.709 22.38 8.05 67.96693 62.21918012 91.54331397

5000 39.82 1.6 21.2 8.05 63.712 55.8310559 87.63036147

10000 39.84 1.37 18.97 8.05 54.5808 44.70321739 81.90282552

12000 39.85 1.271 18.02 8.05 50.64935 40.33793789 79.6415707

15000 39.87 1.129 16.63 8.05 45.01323 34.35489441 76.3217712

20000 39.89 0.945 14.65 8.05 37.69605 26.66118012 70.72672103

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Using an input sine wave with a Vpk−pk of 5.6V:Input Freq. (Hz) Vin (VDC ) Iin (ADC ) Vout (VRMS) Resistance (Ω) Pin (W) Pout (W) Efficiency (%)

20 39.75 2.1 25.14 8.05 83.475 78.51175155 94.05420971

50 39.74 2.093 25.17 8.05 83.17582 78.69924224 94.61793372

100 39.74 2.095 25.17 8.05 83.2553 78.69924224 94.52760633

200 39.74 2.093 25.15 8.05 83.17582 78.5742236 94.46762725

500 39.72 2.092 25.09 8.05 83.09424 78.19976398 94.10972888

1000 39.72 2.085 25 8.05 82.8162 77.63975155 93.7494736

2000 39.73 2.059 24.69 8.05 81.80407 75.7262236 92.5702396

5000 39.75 1.918 23.37 8.05 76.2405 67.84557764 88.98889388

10000 39.8 1.62 20.72 8.05 64.476 53.33147826 82.71524018

12000 39.82 1.506 19.71 8.05 59.96892 48.25889441 80.47317579

15000 39.84 1.323 18.09 8.05 52.70832 40.65193789 77.12622578

20000 39.88 1.09 15.92 8.05 43.4692 31.48402484 72.42835121

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Appendix K

Final Efficiency Test Results

The following appendix gives all the data that was gathered to calculate the efficiency of

the final system. This was done at varying output voltages, clock frequencies and signal

frequencies.

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Freq. (Hz) I12 (A) I5 (A) I−12 (A) Vin (V ) Iin (A) Vout (Vrms) Res. (Ω) Pin−sig. (W) Pin (W) Pout (W) Efficiency PS (%) Efficieny Total (%)

20 0.040 0.012 0.007 39.61 0.15 5.69 8.05 0.62 5.94 4.02 67.69% 61.26%

50 0.040 0.012 0.007 39.61 0.14 5.69 8.05 0.62 5.55 4.02 72.53% 65.19%

100 0.040 0.012 0.007 39.62 0.15 5.69 8.05 0.62 5.94 4.02 67.67% 61.24%

200 0.040 0.012 0.007 39.61 0.14 5.69 8.05 0.62 5.55 4.02 72.53% 65.19%

500 0.045 0.012 0.007 39.61 0.14 5.70 8.05 0.68 5.55 4.04 72.78% 64.79%

1000 0.045 0.012 0.007 39.62 0.15 5.69 8.05 0.68 5.94 4.02 67.67% 60.69%

2000 0.045 0.012 0.007 39.62 0.15 5.71 8.05 0.68 5.94 4.05 68.15% 61.12%

5000 0.045 0.012 0.007 39.62 0.15 5.83 8.05 0.68 5.94 4.22 71.05% 63.71%

10000 0.045 0.012 0.007 39.63 0.16 6.11 8.05 0.68 6.34 4.64 73.14% 66.02%

12000 0.045 0.012 0.007 39.60 0.17 6.20 8.05 0.68 6.73 4.78 70.93% 64.39%

15000 0.045 0.012 0.007 39.60 0.17 6.24 8.05 0.68 6.73 4.84 71.85% 65.22%

20000 0.044 0.012 0.007 39.61 0.17 6.12 8.05 0.67 6.73 4.65 69.10% 62.83%

Vin(Vp−p)

1.08

Freq. (Hz) I12 (A) I5 (A) I−12 (A) Vin (V ) Iin (A) Vout (Vrms) Res. (Ω) Pin−sig. (W) Pin (W) Pout (W) Efficiency PS (%) Efficieny Total (%)

20 0.040 0.014 0.007 39.61 0.60 12.84 8.05 0.63 23.77 20.48 86.17% 83.94%

50 0.041 0.014 0.007 39.61 0.58 12.85 8.05 0.65 22.97 20.51 89.28% 86.84%

100 0.040 0.014 0.007 39.60 0.58 12.86 8.05 0.63 22.97 20.54 89.45% 87.04%

200 0.040 0.012 0.007 39.60 0.58 12.86 8.05 0.62 22.97 20.54 89.45% 87.08%

500 0.039 0.012 0.007 39.61 0.58 12.87 8.05 0.61 22.97 20.58 89.56% 87.24%

1000 0.040 0.012 0.007 39.61 0.58 12.87 8.05 0.62 22.97 20.58 89.56% 87.19%

2000 0.039 0.012 0.007 39.68 0.58 12.88 8.05 0.61 23.01 20.61 89.54% 87.22%

5000 0.040 0.012 0.007 39.60 0.59 12.97 8.05 0.62 23.36 20.90 89.44% 87.11%

10000 0.040 0.012 0.007 39.60 0.61 13.14 8.05 0.62 24.16 21.45 88.79% 86.56%

12000 0.040 0.012 0.007 39.60 0.61 13.16 8.05 0.62 24.16 21.51 89.06% 86.82%

15000 0.040 0.012 0.007 39.60 0.59 13.06 8.05 0.62 23.36 21.19 90.69% 88.33%

20000 0.040 0.012 0.007 39.60 0.55 12.46 8.05 0.62 21.78 19.29 88.55% 86.08%

Vin(Vp−p)

2.5

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Freq. (Hz) I12 (A) I5 (A) I−12 (A) Vin (V ) Iin (A) Vout (Vrms) Res. (Ω) Pin−sig. (W) Pin (W) Pout (W) Efficiency PS (%) Efficieny Total (%)

20 0.030 0.012 0.007 39.56 1.30 20.04 8.05 0.50 51.43 49.89 97.01% 96.06%

50 0.030 0.014 0.007 39.56 1.33 20.06 8.05 0.51 52.61 49.99 95.01% 94.09%

100 0.030 0.014 0.007 39.56 1.33 20.07 8.05 0.51 52.61 50.04 95.10% 94.18%

200 0.030 0.012 0.007 39.55 1.33 20.07 8.05 0.50 52.60 50.04 95.13% 94.22%

500 0.030 0.012 0.007 39.55 1.33 20.07 8.05 0.50 52.60 50.04 95.13% 94.22%

1000 0.030 0.012 0.007 39.55 1.33 20.08 8.05 0.50 52.60 50.09 95.22% 94.32%

2000 0.032 0.012 0.007 39.54 1.33 20.08 8.05 0.53 52.59 50.09 95.25% 94.30%

5000 0.034 0.012 0.007 39.55 1.34 20.13 8.05 0.55 53.00 50.34 94.98% 94.00%

10000 0.034 0.012 0.007 39.54 1.35 20.17 8.05 0.55 53.38 50.54 94.68% 93.71%

12000 0.034 0.012 0.007 39.54 1.35 20.12 8.05 0.55 53.38 50.29 94.21% 93.24%

15000 0.034 0.012 0.007 39.54 1.34 19.96 8.05 0.55 52.98 49.49 93.41% 92.44%

20000 0.034 0.012 0.007 39.55 1.28 19.30 8.05 0.55 50.62 46.27 91.40% 90.42%

Vin(Vp−p)

3.9

Freq. (Hz) I12 (A) I5 (A) I−12 (A) Vin (V ) Iin (A) Vout (Vrms) Res. (Ω) Pin−sig. (W) Pin (W) Pout (W) Efficiency PS (%) Efficieny Total (%)

20 0.030 0.014 0.007 39.65 2.30 26.32 8.05 0.51 91.20 86.05 94.36% 93.83%

50 0.030 0.014 0.007 39.64 2.27 26.34 8.05 0.51 89.98 86.19 95.78% 95.24%

100 0.030 0.014 0.007 39.64 2.27 26.35 8.05 0.51 89.98 86.25 95.85% 95.31%

200 0.030 0.012 0.007 39.64 2.27 26.35 8.05 0.50 89.98 86.25 95.85% 95.32%

500 0.030 0.012 0.007 39.65 2.27 26.36 8.05 0.50 90.01 86.32 95.90% 95.37%

1000 0.030 0.012 0.007 39.64 2.27 26.37 8.05 0.50 89.98 86.38 96.00% 95.46%

2000 0.031 0.012 0.007 39.64 2.27 26.39 8.05 0.52 89.98 86.51 96.14% 95.60%

5000 0.029 0.012 0.007 39.64 2.28 26.40 8.05 0.49 90.38 86.58 95.80% 95.28%

10000 0.029 0.012 0.007 39.64 2.30 26.45 8.05 0.49 91.17 86.91 95.32% 94.81%

12000 0.029 0.012 0.007 39.63 2.35 26.64 8.05 0.49 93.13 88.16 94.66% 94.17%

15000 0.028 0.012 0.007 39.62 2.38 26.78 8.05 0.48 94.30 89.09 94.48% 94.00%

20000 0.021 0.014 0.008 39.60 2.71 28.53 8.05 0.42 107.32 101.11 94.22% 93.85%

Vin(Vp−p)

5.1

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Freq. (Hz) I12 (A) I5 (A) I−12 (A) Vin (V ) Iin (A) Vout (Vrms) Res. (Ω) Pin−sig. (W) Pin (W) Pout (W) Efficiency PS (%) Efficieny Total (%)

20 0.070 0.013 0.006 39.84 0.20 6.96 8.05 0.98 7.97 6.02 75.52% 67.27%

50 0.060 0.013 0.006 39.85 0.20 6.94 8.05 0.86 7.97 5.98 75.07% 67.78%

100 0.060 0.130 0.006 39.85 0.20 6.94 8.05 1.44 7.97 5.98 75.07% 63.57%

200 0.060 0.013 0.006 39.85 0.21 6.94 8.05 0.86 8.37 5.98 71.49% 64.85%

500 0.060 0.013 0.006 39.85 0.20 6.94 8.05 0.86 7.97 5.98 75.07% 67.78%

1000 0.060 0.013 0.006 39.85 0.20 6.95 8.05 0.86 7.97 6.00 75.29% 67.98%

2000 0.059 0.013 0.006 39.85 0.20 6.96 8.05 0.85 7.97 6.02 75.50% 68.27%

5000 0.062 0.013 0.006 39.85 0.20 7.00 8.05 0.88 7.97 6.09 76.37% 68.77%

10000 0.066 0.013 0.006 39.85 0.23 7.26 8.05 0.93 9.17 6.55 71.44% 64.86%

12000 0.067 0.013 0.006 39.84 0.24 7.37 8.05 0.94 9.56 6.75 70.57% 64.25%

15000 0.067 0.013 0.006 39.84 0.25 7.45 8.05 0.94 9.96 6.89 69.22% 63.25%

20000 0.067 0.013 0.006 39.85 0.23 7.26 8.05 0.94 9.17 6.55 71.44% 64.79%

Vin(Vp−p)

1.4

Freq. (Hz) I12 (A) I5 (A) I−12 (A) Vin (V ) Iin (A) Vout (Vrms) Res. (Ω) Pin−sig. (W) Pin (W) Pout (W) Efficiency PS (%) Efficieny Total (%)

20 0.060 0.013 0.006 39.80 0.63 13.55 8.05 0.86 25.07 22.81 90.96% 87.96%

50 0.055 0.013 0.006 39.80 0.64 13.56 8.05 0.80 25.47 22.84 89.67% 86.95%

100 0.055 0.013 0.006 39.80 0.64 13.57 8.05 0.80 25.47 22.88 89.81% 87.08%

200 0.055 0.013 0.006 39.79 0.64 13.56 8.05 0.80 25.47 22.84 89.70% 86.97%

500 0.055 0.013 0.007 39.80 0.64 13.57 8.05 0.81 25.47 22.88 89.81% 87.04%

1000 0.055 0.014 0.007 39.79 0.64 13.57 8.05 0.81 25.47 22.88 89.83% 87.05%

2000 0.055 0.014 0.006 39.80 0.64 13.59 8.05 0.80 25.47 22.94 90.07% 87.32%

5000 0.059 0.014 0.007 39.79 0.65 13.65 8.05 0.86 25.86 23.15 89.49% 86.61%

10000 0.058 0.014 0.007 39.78 0.68 13.84 8.05 0.85 27.05 23.79 87.96% 85.28%

12000 0.058 0.014 0.007 39.78 0.68 13.86 8.05 0.85 27.05 23.86 88.22% 85.53%

15000 0.058 0.014 0.007 39.78 0.68 13.80 8.05 0.85 27.05 23.66 87.46% 84.79%

20000 0.057 0.014 0.007 39.79 0.63 13.18 8.05 0.84 25.07 21.58 86.08% 83.30%

Vin(Vp−p)

2.7

134

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Freq. (Hz) I12 (A) I5 (A) I−12 (A) Vin (V ) Iin (A) Vout (Vrms) Res. (Ω) Pin−sig. (W) Pin (W) Pout (W) Efficiency PS (%) Efficieny Total (%)

20 0.045 0.013 0.007 39.70 1.60 22.10 8.05 0.69 63.52 60.67 95.52% 94.49%

50 0.045 0.013 0.007 39.69 1.62 22.12 8.05 0.69 64.30 60.78 94.53% 93.53%

100 0.045 0.013 0.007 39.69 1.62 22.13 8.05 0.69 64.30 60.84 94.62% 93.61%

200 0.045 0.013 0.070 39.70 1.62 22.13 8.05 1.45 64.31 60.84 94.59% 92.51%

500 0.045 0.013 0.007 39.70 1.62 22.13 8.05 0.69 64.31 60.84 94.59% 93.59%

1000 0.045 0.013 0.007 39.69 1.62 22.15 8.05 0.69 64.30 60.95 94.79% 93.78%

2000 0.043 0.013 0.007 39.70 1.62 22.16 8.05 0.67 64.31 61.00 94.85% 93.88%

5000 0.047 0.013 0.007 39.71 1.63 22.18 8.05 0.71 64.73 61.11 94.41% 93.39%

10000 0.046 0.013 0.007 39.70 1.64 22.16 8.05 0.70 65.11 61.00 93.69% 92.70%

12000 0.046 0.013 0.007 39.71 1.63 22.05 8.05 0.70 64.73 60.40 93.31% 92.31%

15000 0.045 0.013 0.007 39.71 1.59 21.71 8.05 0.69 63.14 58.55 92.73% 91.73%

20000 0.044 0.013 0.007 39.70 1.46 20.57 8.05 0.68 57.96 52.56 90.68% 89.64%

Vin(Vp−p)

4.34

Freq. (Hz) I12 (A) I5 (A) I−12 (A) Vin (V ) Iin (A) Vout (Vrms) Res. (Ω) Pin−sig. (W) Pin (W) Pout (W) Efficiency PS (%) Efficieny Total (%)

20 0.040 0.013 0.007 39.64 2.30 26.61 8.05 0.63 91.17 87.96 96.48% 95.82%

50 0.040 0.013 0.007 39.64 2.33 26.64 8.05 0.63 92.36 88.16 95.45% 94.81%

100 0.040 0.013 0.007 39.63 2.33 26.64 8.05 0.63 92.34 88.16 95.48% 94.83%

200 0.040 0.013 0.007 39.63 2.33 26.64 8.05 0.63 92.34 88.16 95.48% 94.83%

500 0.040 0.013 0.007 39.63 2.32 26.65 8.05 0.63 91.94 88.23 95.96% 95.31%

1000 0.040 0.012 0.007 39.64 2.33 26.67 8.05 0.62 92.36 88.36 95.67% 95.02%

2000 0.036 0.013 0.007 39.64 2.33 26.68 8.05 0.58 92.36 88.43 95.74% 95.14%

5000 0.040 0.013 0.007 39.64 2.34 26.67 8.05 0.63 92.76 88.36 95.26% 94.62%

10000 0.040 0.012 0.007 39.65 2.33 26.53 8.05 0.62 92.38 87.43 94.64% 94.01%

12000 0.040 0.013 0.007 39.66 2.32 26.41 8.05 0.63 92.01 86.64 94.17% 93.53%

15000 0.038 0.013 0.007 39.66 2.34 26.42 8.05 0.61 92.80 86.71 93.43% 92.83%

20000 0.034 0.013 0.007 39.67 2.26 25.87 8.05 0.56 89.65 83.14 92.73% 92.16%

Vin(Vp−p)

5.2

135

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Freq. (Hz) I12 (A) I5 (A) I−12 (A) Vin (V ) Iin (A) Vout (Vrms) Res. (Ω) Pin−sig. (W) Pin (W) Pout (W) Efficiency PS (%) Efficieny Total (%)

20 0.060 0.014 0.007 39.85 0.18 6.81 8.05 0.87 7.17 5.76 80.32% 71.59%

50 0.060 0.014 0.007 39.85 0.18 6.81 8.05 0.87 7.17 5.76 80.32% 71.59%

100 0.060 0.014 0.006 39.85 0.18 6.82 8.05 0.86 7.17 5.78 80.55% 71.91%

200 0.060 0.014 0.006 39.85 0.18 6.82 8.05 0.86 7.17 5.78 80.55% 71.91%

500 0.060 0.014 0.006 39.85 0.18 6.82 8.05 0.86 7.17 5.78 80.55% 71.91%

1000 0.060 0.014 0.006 39.85 0.18 6.82 8.05 0.86 7.17 5.78 80.55% 71.91%

2000 0.058 0.014 0.006 39.85 0.18 6.82 8.05 0.84 7.17 5.78 80.55% 72.13%

5000 0.055 0.014 0.006 39.85 0.18 6.81 8.05 0.80 7.17 5.76 80.32% 72.24%

10000 0.055 0.014 0.006 39.85 0.18 6.75 8.05 0.80 7.17 5.66 78.91% 70.97%

12000 0.055 0.014 0.006 39.85 0.18 6.70 8.05 0.80 7.17 5.58 77.74% 69.92%

15000 0.055 0.014 0.006 39.85 0.17 6.56 8.05 0.80 6.77 5.35 78.91% 70.56%

20000 0.055 0.014 0.006 39.86 0.16 6.12 8.05 0.80 6.38 4.65 72.95% 64.80%

Vin(Vp−p)

1.38

Freq. (Hz) I12 (A) I5 (A) I−12 (A) Vin (V ) Iin (A) Vout (Vrms) Res. (Ω) Pin−sig. (W) Pin (W) Pout (W) Efficiency PS (%) Efficieny Total (%)

20 0.080 0.014 0.007 39.81 0.60 13.22 8.05 1.11 23.89 21.71 90.89% 86.84%

50 0.060 0.014 0.007 39.81 0.60 13.22 8.05 0.87 23.89 21.71 90.89% 87.68%

100 0.060 0.014 0.007 39.83 0.60 13.22 8.05 0.87 23.90 21.71 90.85% 87.64%

200 0.060 0.014 0.007 39.82 0.60 13.22 8.05 0.87 23.89 21.71 90.87% 87.66%

500 0.060 0.014 0.007 39.82 0.60 13.21 8.05 0.87 23.89 21.68 90.73% 87.53%

1000 0.060 0.014 0.006 39.82 0.60 13.21 8.05 0.86 23.89 21.68 90.73% 87.57%

2000 0.060 0.014 0.006 39.81 0.60 13.21 8.05 0.86 23.89 21.68 90.75% 87.59%

5000 0.060 0.014 0.006 39.82 0.62 13.29 8.05 0.86 24.69 21.94 88.87% 85.87%

10000 0.056 0.014 0.006 39.82 0.62 13.40 8.05 0.81 24.81 22.31 89.91% 87.06%

12000 0.060 0.014 0.006 39.82 0.63 13.37 8.05 0.86 25.09 22.21 88.52% 85.58%

15000 0.600 0.014 0.006 39.82 0.63 13.34 8.05 7.34 25.09 22.11 88.12% 68.17%

20000 0.060 0.014 0.007 39.82 0.61 13.13 8.05 0.87 24.29 21.42 88.17% 85.10%

Vin(Vp−p)

2.66

136

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Freq. (Hz) I12 (A) I5 (A) I−12 (A) Vin (V ) Iin (A) Vout (Vrms) Res. (Ω) Pin−sig. (W) Pin (W) Pout (W) Efficiency PS (%) Efficieny Total (%)

20 0.060 0.014 0.007 39.78 1.60 21.82 8.05 0.87 63.65 59.14 92.92% 91.67%

50 0.050 0.014 0.007 39.78 1.57 21.84 8.05 0.75 62.45 59.25 94.87% 93.74%

100 0.050 0.014 0.007 39.78 1.57 21.84 8.05 0.75 62.45 59.25 94.88% 93.75%

200 0.050 0.014 0.007 39.78 1.57 21.84 8.05 0.75 62.45 59.25 94.87% 93.74%

500 0.050 0.014 0.007 39.77 1.57 21.84 8.05 0.75 62.44 59.25 94.90% 93.77%

1000 0.050 0.014 0.007 39.77 1.58 21.85 8.05 0.75 62.84 59.31 94.38% 93.26%

2000 0.050 0.014 0.007 39.78 1.58 21.87 8.05 0.75 62.85 59.42 94.53% 93.41%

5000 0.047 0.014 0.007 39.78 1.58 21.88 8.05 0.72 62.85 59.47 94.62% 93.55%

10000 0.049 0.014 0.007 39.77 1.60 21.88 8.05 0.74 63.63 59.47 93.46% 92.38%

12000 0.048 0.014 0.007 39.77 1.59 21.79 8.05 0.73 63.23 58.98 93.28% 92.21%

15000 0.047 0.014 0.007 39.77 1.56 21.48 8.05 0.72 62.04 57.32 92.38% 91.33%

20000 0.047 0.014 0.007 39.78 1.40 20.19 8.05 0.72 55.69 50.64 90.93% 89.77%

Vin(Vp−p)

4.3

Freq. (Hz) I12 (A) I5 (A) I−12 (A) Vin (V ) Iin (A) Vout (Vrms) Res. (Ω) Pin−sig. (W) Pin (W) Pout (W) Efficiency PS (%) Efficieny Total (%)

20 0.050 0.014 0.006 39.67 2.30 26.57 8.05 0.74 91.24 87.70 96.12% 95.34%

50 0.050 0.014 0.007 39.67 2.31 26.59 8.05 0.75 91.64 87.83 95.84% 95.06%

100 0.050 0.014 0.007 39.67 2.31 26.60 8.05 0.75 91.64 87.90 95.92% 95.13%

200 0.040 0.014 0.007 39.67 2.31 26.59 8.05 0.63 91.64 87.83 95.84% 95.19%

500 0.050 0.014 0.007 39.68 2.31 26.60 8.05 0.75 91.66 87.90 95.89% 95.11%

1000 0.050 0.014 0.007 39.68 2.31 26.62 8.05 0.75 91.66 88.03 96.04% 95.25%

2000 0.040 0.014 0.007 39.80 2.33 26.71 8.05 0.63 92.73 88.62 95.57% 94.92%

5000 0.040 0.014 0.007 39.75 2.32 26.64 8.05 0.63 92.22 88.16 95.60% 94.94%

10000 0.041 0.014 0.007 39.76 2.32 26.51 8.05 0.65 92.24 87.30 94.64% 93.98%

12000 0.041 0.014 0.007 39.75 2.30 26.29 8.05 0.65 91.43 85.86 93.91% 93.25%

15000 0.040 0.014 0.007 39.76 2.25 25.94 8.05 0.63 89.46 83.59 93.44% 92.78%

20000 0.036 0.014 0.007 39.77 2.14 25.17 8.05 0.59 85.11 78.70 92.47% 91.84%

Vin(Vp−p)

5.2

137

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Freq. (Hz) I12 (A) I5 (A) I−12 (A) Vin (V ) Iin (A) Vout (Vrms) Res. (Ω) Pin−sig. (W) Pin (W) Pout (W) Efficiency PS (%) Efficieny Total (%)

20 0.060 0.016 0.007 39.66 0.15 6.36 8.05 0.88 5.95 5.02 84.46% 73.54%

50 0.060 0.016 0.007 39.67 0.16 6.37 8.05 0.88 6.35 5.04 79.41% 69.71%

100 0.060 0.016 0.007 39.66 0.16 6.37 8.05 0.88 6.35 5.04 79.43% 69.72%

200 0.060 0.016 0.007 39.66 0.16 6.37 8.05 0.88 6.35 5.04 79.43% 69.72%

500 0.060 0.016 0.007 39.66 0.16 6.37 8.05 0.88 6.35 5.04 79.43% 69.72%

1000 0.060 0.016 0.007 39.66 0.16 6.37 8.05 0.88 6.35 5.04 79.43% 69.72%

2000 0.060 0.016 0.007 39.66 0.16 6.37 8.05 0.88 6.35 5.04 79.43% 69.72%

5000 0.060 0.016 0.007 39.65 0.16 6.35 8.05 0.88 6.34 5.01 78.96% 69.30%

10000 0.058 0.016 0.007 39.65 0.16 6.28 8.05 0.86 6.34 4.90 77.23% 68.01%

12000 0.058 0.016 0.007 39.64 0.16 6.22 8.05 0.86 6.34 4.81 75.78% 66.73%

15000 0.058 0.016 0.007 39.64 0.16 6.06 8.05 0.86 6.34 4.56 71.93% 63.34%

20000 0.056 0.016 0.007 39.63 0.14 5.64 8.05 0.84 5.55 3.95 71.22% 61.90%

Vin(Vp−p)

1.31

Freq. (Hz) I12 (A) I5 (A) I−12 (A) Vin (V ) Iin (A) Vout (Vrms) Res. (Ω) Pin−sig. (W) Pin (W) Pout (W) Efficiency PS (%) Efficieny Total (%)

20 0.060 0.016 0.007 39.63 0.60 13.29 8.05 0.88 23.78 21.94 92.27% 88.97%

50 0.060 0.016 0.007 39.63 0.62 13.30 8.05 0.88 24.57 21.97 89.43% 86.33%

100 0.060 0.016 0.007 39.63 0.62 13.31 8.05 0.88 24.57 22.01 89.57% 86.46%

200 0.060 0.016 0.007 39.63 0.62 13.31 8.05 0.88 24.57 22.01 89.57% 86.46%

500 0.060 0.016 0.007 39.63 0.62 13.31 8.05 0.88 24.57 22.01 89.57% 86.46%

1000 0.060 0.016 0.007 39.63 0.62 13.31 8.05 0.88 24.57 22.01 89.57% 86.46%

2000 0.058 0.016 0.007 39.63 0.62 13.34 8.05 0.86 24.57 22.11 89.97% 86.93%

5000 0.055 0.016 0.007 39.63 0.62 13.41 8.05 0.82 24.57 22.34 90.92% 87.97%

10000 0.062 0.016 0.007 39.61 0.64 13.49 8.05 0.91 25.35 22.61 89.18% 86.09%

12000 0.063 0.016 0.007 39.62 0.65 13.46 8.05 0.92 25.75 22.51 87.39% 84.38%

15000 0.062 0.016 0.007 39.62 0.66 13.53 8.05 0.91 26.15 22.74 86.96% 84.05%

20000 0.060 0.016 0.007 39.61 0.63 13.23 8.05 0.88 24.95 21.74 87.13% 84.15%

Vin

2.69

138

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Freq. (Hz) I12 (A) I5 (A) I−12 (A) Vin (V ) Iin (A) Vout (Vrms) Res. (Ω) Pin−sig. (W) Pin (W) Pout (W) Efficiency PS (%) Efficieny Total (%)

20 0.050 0.016 0.007 39.54 1.40 20.19 8.05 0.76 55.36 50.64 91.48% 90.23%

50 0.060 0.016 0.007 39.54 1.36 20.20 8.05 0.88 53.77 50.69 94.26% 92.74%

100 0.060 0.016 0.007 39.56 1.36 20.21 8.05 0.88 53.80 50.74 94.31% 92.78%

200 0.060 0.016 0.007 39.56 1.37 20.21 8.05 0.88 54.20 50.74 93.62% 92.12%

500 0.050 0.016 0.007 39.57 1.37 20.22 8.05 0.76 54.21 50.79 93.69% 92.39%

1000 0.050 0.016 0.007 39.55 1.37 20.22 8.05 0.76 54.18 50.79 93.73% 92.43%

2000 0.050 0.016 0.007 39.54 1.37 20.24 8.05 0.76 54.17 50.89 93.94% 92.64%

5000 0.052 0.016 0.007 39.55 1.37 20.26 8.05 0.79 54.18 50.99 94.11% 92.76%

10000 0.053 0.016 0.007 39.56 1.39 20.29 8.05 0.80 54.99 51.14 93.00% 91.67%

12000 0.053 0.016 0.007 39.55 1.39 20.25 8.05 0.80 54.97 50.94 92.66% 91.33%

15000 0.053 0.016 0.007 39.55 1.37 19.98 8.05 0.80 54.18 49.59 91.52% 90.19%

20000 0.050 0.016 0.007 39.57 1.23 18.77 8.05 0.76 48.67 43.77 89.92% 88.53%

Vin(Vp−p)

4.02

Freq. (Hz) I12 (A) I5 (A) I−12 (A) Vin (V ) Iin (A) Vout (Vrms) Res. (Ω) Pin−sig. (W) Pin (W) Pout (W) Efficiency PS (%) Efficieny Total (%)

20 0.060 0.016 0.007 39.45 2.30 26.62 8.05 0.88 90.74 88.03 97.02% 96.08%

50 0.050 0.016 0.007 39.43 2.34 26.65 8.05 0.76 92.27 88.23 95.62% 94.84%

100 0.050 0.016 0.007 39.46 2.34 26.66 8.05 0.76 92.34 88.29 95.62% 94.84%

200 0.040 0.016 0.007 39.43 2.34 26.65 8.05 0.64 92.27 88.23 95.62% 94.96%

500 0.040 0.016 0.007 39.43 2.34 26.66 8.05 0.64 92.27 88.29 95.69% 95.03%

1000 0.040 0.016 0.007 39.42 2.34 26.68 8.05 0.64 92.24 88.43 95.86% 95.20%

2000 0.040 0.016 0.007 39.41 2.34 26.69 8.05 0.64 92.22 88.49 95.96% 95.29%

5000 0.044 0.016 0.007 39.42 2.35 26.64 8.05 0.69 92.64 88.16 95.17% 94.46%

10000 0.043 0.016 0.007 39.43 2.34 26.51 8.05 0.68 92.27 87.30 94.62% 93.93%

12000 0.042 0.016 0.007 39.44 2.32 26.33 8.05 0.67 91.50 86.12 94.12% 93.44%

15000 0.040 0.016 0.007 39.41 2.29 26.04 8.05 0.64 90.25 84.23 93.33% 92.67%

20000 0.036 0.016 0.007 39.45 2.17 25.32 8.05 0.60 85.61 79.64 93.03% 92.39%

Vin(Vp−p)

5.25

139

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Appendix L

Final Sound Quality Test Results

The following appendix gives all the plots that were taken for sound quality testing. These

include Total Harmonic Distortion, Signal to Noise Ratio and Frequency Response. First

the loopback results are shown. Then those that were taken by sweeping through input

frequencies and using a 1MHz, 2MHz, 5MHz, and 10MHz clock frequencies are given

140

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L.1 Loopback Results

101

102

103

104

105

1

2

3

4

5

6

7

8

9

10x 10

−3 THD vs Frequency (Loopback)

Signal Frequency (Hz)

TH

D (

%)

Figure L.1: THD results for Loopback Test

101

102

103

104

105

−0.07

−0.06

−0.05

−0.04

−0.03

−0.02

−0.01

0Frequency Response (Loopback)

Signal Frequency (Hz)

Am

plitu

de (

dB)

with

1kH

z R

efer

ence

Figure L.2: Frequency Response results for Loopback Test

141

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L.2 Signal Quality Results with 1MHz Modulation Fre-

quency

101

102

103

104

105

4

5

6

7

8

9

10

11THD vs Frequency at 1MHz Modulation Frequency

Signal Frequency (Hz)

TH

D (

%)

Figure L.3: THD results at 1MHz clock frequency

101

102

103

104

105

77.5

77.6

77.7

77.8

77.9

78

78.1

78.2

78.3

78.4

78.5SNR vs Frequency at 1MHz Modulation Frequency

Signal Frequency (Hz)

SN

R (

dB)

Figure L.4: SNR results at 1MHz clock frequency

142

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101

102

103

104

105

−0.8

−0.7

−0.6

−0.5

−0.4

−0.3

−0.2

−0.1

0

0.1

0.2Frequency Response at 1MHz Modulation Frequency

Signal Frequency (Hz)

Am

plitu

de (

dB)

with

1kH

z R

efer

ence

Figure L.5: Frequency Response resuplotlts at 1MHz clock frequency

L.3 Signal Quality Results with 2MHz Modulation Fre-

quency

101

102

103

104

105

5

6

7

8

9

10

11

12THD vs Frequency at 2MHz Modulation Frequency

Signal Frequency (Hz)

TH

D (

%)

Figure L.6: THD results at 2MHz clock frequency

143

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101

102

103

104

105

83

83.2

83.4

83.6

83.8

84

84.2

84.4

84.6SNR vs Frequency at 2MHz Modulation Frequency

Signal Frequency (Hz)

SN

R (

dB)

Figure L.7: SNR results at 2MHz clock frequency

101

102

103

104

105

5

6

7

8

9

10

11

12THD vs Frequency at 2MHz Modulation Frequency

Signal Frequency (Hz)

TH

D (

%)

Figure L.8: Frequency Response results at 2MHz clock frequency

144

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L.4 Signal Quality Results with 5MHz Modulation Fre-

quency

101

102

103

104

0

0.2

0.4

0.6

0.8

1

1.2

1.4

1.6

1.8

2THD vs Frequency at 5MHz Modulation Frequency

Signal Frequency (Hz)

TH

D (

%)

Figure L.9: THD results at 5MHz clock frequency

101

102

103

104

105

89

89.5

90

90.5

91

91.5

92

92.5SNR vs Frequency at 5MHz Modulation Frequency

Signal Frequency (Hz)

SN

R (

dB)

Figure L.10: SNR results at 5MHz clock frequency

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101

102

103

104

105

−3

−2.5

−2

−1.5

−1

−0.5

0Frequency Response at 5MHz Modulation Frequency

Signal Frequency (Hz)

Am

plitu

de (

dB)

with

1kH

z R

efer

ence

Figure L.11: Frequency Response results at 5MHz clock frequency

L.5 Signal Quality Results with 10MHz Modulation

Frequency

101

102

103

104

0

0.2

0.4

0.6

0.8

1

1.2

1.4

1.6

1.8

2THD vs Frequency at 10MHz Modulation Frequency

Signal Frequency (Hz)

TH

D (

%)

Figure L.12: THD results at 10MHz clock frequency

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101

102

103

104

105

86.5

87

87.5

88

88.5

89

89.5

90

90.5

91

91.5SNR vs Frequency at 10MHz Modulation Frequency

Signal Frequency (Hz)

SN

R (

dB)

Figure L.13: SNR results at 10MHz clock frequency

101

102

103

104

105

−5

−4.5

−4

−3.5

−3

−2.5

−2

−1.5

−1

−0.5

0Frequency Response at 10MHz Modulation Frequency

Signal Frequency (Hz)

Am

plitu

de (

dB)

with

1kH

z R

efer

ence

Figure L.14: Frequency Response results at 10MHz clock frequency

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Appendix M

Digital Audio

Digital audio has been around in various forms for over 20 years, the most ubiquitous form

being the Compact Disc (CD) format. In more recent years digital audio has moved to other

media, such as the Internet, and digital audio players, such as iPods. All of the advances

in digital audio have greatly benefitted consumers, especially those interested in hi-fidelity

sound systems. The live audio market however, has remained mostly in the analog domain,

specifically with regard to live audio mixing consoles and amplifiers. In some respects this

makes sense; the purpose of live audio equipment is to amplify an analog signal for immediate

playback, so converting to digital seems like it would be a cumbersome step that would

introduce more problems than it would solve. With recent advances in technology, however,

the hurdles associated with digital audio, such as increased noise and decreased audio fidelity,

have almost been completely negated.

Before beginning a discussion of the way in which digital audio could be implemented in

the live audio market, several terms need to be defined. The quality of a digital audio signal

can be described by numbers, most importantly the sampling frequency, or Nyquist Rate, and

the bit depth. The sampling frequency is how often a single digital sample is taken from the

analog signal. A Nyquist Rate of 96 kHz means that one second of audio has 96,000 samples.

This number is important because the Nyquist-Shannon Sampling Theorem dictates how

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much bandwidth a digital system can capture. According to the theorem a system must

sample at a rate a frequency of at least twice the highest frequency in the original signal

(the Nyquist Frequency); however, most systems for digital audio oversample anywhere from

44.1 kHz (CDs) to 96 kHz, especially for high end digital mixing consoles. A small amount

of oversampling is necessary to counter real world non-idealities such as imperfect filters,

though in practice the amount of oversampling required is minimal at perhaps 2.2 times the

Nyquist Frequency instead of twice the Nyquist Frequency. While high end digital audio

has Nyquist Rates of up to 96 kHz, significantly higher than the required Nyquist Rate, it is

difficult to experimentally prove this rate is necessary. Regardless of technical reasons, the

market expects a higher Nyquist Rate for high end digital audio, so engineers must meet

market expectations for products to be successful.

The bit depth, how many bits per sample, is somewhat more important for audio quality.

A CD has a bit depth of 16 bits per sample, which means that there are 216 different possible

values for each individual sample. These values correspond to the analog voltage level of

the original signal. The limiting factor of 16 bit audio is the maximum dynamic range, or

the maximum difference between the loudest and quietest sound that a system can produce.

16 bit audio is limited to a 96 dB maximum dynamic range, though CDs rarely achieve

this total range. While 96 dB may seem like an adequate dynamic range for audio, many

bands require sound levels of over 110 dB in their venues. A maximum dynamic range of

only 96 dB would therefore result in a relatively loud noise floor, manifested as a hissing

during quiet portions of the show. The solution to this problem is to move to 24 bits per

sample, which has a maximum dynamic range of 144 dB. The threshold of pain is roughly

125 dB, so a dynamic range of 144 dB is more than adequate for providing high quality

sound with minimal noise in live audio. The first step towards digital audio in the live audio

market was the development of digital mixing consoles. There are a number of different

digital mixing consoles produced by a variety of different manufacturers, including Midas, a

company known for producing the some of the highest quality analog mixing consoles. While

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each digital mixing console is different, they all have the same basic operation. An analog

input, such as a microphone or a guitar, is converted to a digital signal through an Analog

to Digital Converter. The digital signal can then be processed in a myriad of different ways,

including features like gating, compressing, and equalizing, that comparable analog mixing

consoles cannot do on-board. Finally, the mixed digital signals are then passed through a

Digital to Analog Converter to be sent to the amplifiers. An immediate benefit can be seen

by the processing options available to a digital mixing console, though some audio purists

argue that the act of converting between digital and audio will degrade the quality of the

signal. Digital mixing consoles sample at rates between 44.1 kHz [YMH07] and 96 kHz

and 24 bits per sample, however [MDS08]. As explained above, these values are more than

adequate to capture any audio during a live concert.

The second link in the chain for a full digital signal path is the snake. A snake is a large

cable that contains multiple audio channels, and is used to easily send signals between the

stage and the mixing console. Traditionally audio snakes have been purely analog, consisting

of many separate audio paths within one large shielded cable. This analog method works and

is still used extensively, but it is expensive to produce the cable, difficult to use because of the

girth of the cable, and potentially subject to noise if the shielding is improperly connected or

grounding issues occur. In comparison, a digital snake is generally a single CAT5 or CAT6

twisted pair cable, the same as used in most personal computer networks. A digital snake

does necessitate Analog to Digital and Digital to Analog converters on either side of the

CAT5/6 cable, but the CAT5/6 cable can be run for up to 330 ft with no repeaters [AES05],

and is virtually immune to any type of noise, including noise caused through improper

grounding or crosstalk. Professional digital snakes use sample rates from 48 kHz to 192 kHz

[SNY08] and sample at 24 bits per second, allowing for capture of signals in the 20 Hz 20

kHz audio band.

Digital mixing consoles and digital audio snakes have both been around for several years,

but they are produced by different manufacturers, and these manufacturers have had little

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incentive to integrate their technology. While this did not lead to technical problems in

mixing for a live audio event, converting back and forth between digital and analog domains

had the potential to add in noise. This argument was valid years ago, but current technology

allows audio engineers to minimize the number of conversions while taking advantage of the

benefits offered by digital audio. One such example is the work between Yamaha, a digital

mixing console manufacturer, and Aviom, a digital audio snake producer. Yamaha designed

some of their digital mixing consoles with expansion ports, for both Yamaha peripherals as

well as third party peripherals. Aviom designed an expansion card that plugs into a Yamaha

digital mixing console and provides a direct digital interface between Avioms digital audio

snake products and Yamahas digital mixing console [AVM08].

Directly interfacing a digital audio snake to a digital mixing console has a number of

benefits, the most obvious being the reduction of the number of conversions between analog

and digital. Another benefit is that plugging a digital audio snake directly into the digital

mixing console reduces the amount of work required to setup for a show, and more impor-

tantly eliminates a major problem area for troubleshooting. When using analog audio, each

channel has a separate connector, and it can be very easy to accidentally swap channels

when connecting everything to the mixing console and effects processors. Since a digital

audio snake is only a single CAT 5/6 cable the chances of accidentally plugging the cable

into the wrong port are greatly minimized.

While the input to a digital mixing console is beginning to move towards all-digital, the

output, or returns, which provide a signal to the amplifiers, remains in the analog domain.

This can be seen by looking at various amplifier specification sheets and talking to audio

engineers. Most audio amplifiers operate in the analog domain, directly amplifying an input

voltage to provide a high power signal to a speaker. For these amplifiers it is necessary

to convert to an analog signal before amplifying; otherwise the amplifier will be unable to

decode a digital signal. The Class D audio amplifier, however, is designed to use MOSFETs

for switching, which is much more efficient. This switching behavior is generally controlled by

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either a Pulse Width Modulator (PWM) or Delta Sigma Modulator, two different modulation

schemes that produce, at a minimum, a two state digital signal that can be used to control

the MOSFETs. Unfortunately, the term digital is very broad, and leads to some incorrect

assumptions. The most important thing to realize is that digital audio cannot be directly

amplified by a digital amplifier. The characteristics of the signals are very different, a digital

audio snake would actually contain anywhere from 16 to 384 audio channels in one direction,

but a Class D audio amplifier is looking for a single audio signal in a PWM-type format. A

special converter module would be required in place of a standard modulator to single out a

specific channel and translate the signal into something the amplifier could use.

It is necessary to deviate slightly to explain how a digital audio snake works to understand

where a project would need to begin to develop a converter module for a digital interface for

a Class D audio amplifier. While a digital audio snake manufacturer could develop their own

proprietary cabling, as mentioned above, most manufacturers choose to use existing technol-

ogy, most notably CAT5 cabling, the same as that used in computer networks around the

globe. Aviom only uses the Physical Layer, as defined by the Open Systems Interconnection

Basic Reference Model (OSI Model), which consists only of the actual hardware that links

two devices together. It is difficult to determine how much more of the OSI Model Aviom

uses, however, as the second layer, the Data Link Layer, handles routing and error correction,

which may be of limited use in a digital audio snake system. As it is impossible to determine

exactly how Avioms system works, it is difficult to provide a starting point for creating a

converter module. Unfortunately Avioms A-Net standard is a closed, proprietary standard,

so while it is easy to understand from a system level, it would be difficult to reverse engineer

the standard.

While it is difficult to be sure of the protocol specifics, some generalizations can be made

based on available technology. A quick primer on network traffic is useful in understanding

how Avioms digital snake might work. Traffic on the internet is divided into two major

protocols, User Datagram Protocol (UDP) and Transmission Control Protocol (TCP). TCP

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is used for applications in which data integrity is paramount, and there is time to resend lost

or damaged packets. One example would be viewing a webpage; this is not a time sensitive

action, so a web browser can request the server resend any missing packets. The other

protocol, UDP, is less reliable, but eschews data integrity for speed. A real-time application,

such as live audio through a digital audio snake, does not have time to resend dropped

packets; it must be capable of handling dropped packets without problem. It should be

noted that since a digital audio snake is an isolated and highly controlled environment, a

connectionless protocol like UDP would probably not drop a significant number of packets,

if any. Even if it did drop a packet, there is no way the system could recognize the missing

information and resend it in time without instituting a delay, which is impossible for live

audio.

Another digital snake standard is called AES50-2005, and is based off of a standard known

as SuperMAC/HyperMAC developed by Sony Pro-Audio Labs [SNY08]. This standard is

an open standard published by the Audio Engineering Society (AES) and designed for High-

Resolution Multi-Channel Audio Interconnection (HRMAI), or in more common terms, a

digital audio snake. Similar to Aviom, AES50-2005 uses CAT5/6 cabling as a physical layer

[AES05]. One digital mixing console that has support for AES50-2005 is the Midas XL8,

Midas Consoles first digital mixing console [MDS08]. The AES50-2005 standard is very well

documented, which would be essential for developing an amplifier that would be capable

of reading and converting an AES50-2005 audio stream. What is interesting about the

AES50-2005 standard is that it uses a specially designed protocol, similar to TCP/UDP, but

designed to function at a lower OSI level and minimize overhead. By reducing the amount

of processing per frame the latency of the system is increased, which is one of the most

important factors for live audio. Another benefit of AES50-2005 is that the individual audio

streams are encoded using Pulse-Code Modulation (PCM), the advantages from PCM will

be explained below [AES05].

Due to the proprietary nature of Avioms protocol, any project focusing on digital audio

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should concentrate on the open AES50-2005 standard. Since the information here is relatively

generic, most of it should apply to Avioms A-Net standard, but it is impossible to be certain

as A-Net is a closed standard. The first step to amplifying digital audio is to develop a

decoder, a subsystem that can read AES50-2005 (or A-Net) protocol. This would require a

transceiver linked to some sort of microprocessor to tune into the proper audio channel. An

excellent solution to this problem would be an embedded real-time Linux system. The I/O

system block would only have to read in the AES50-2005 audio streams and output a single

PCM audio stream. Some sort of user interface would be require to select the channel to

amplify, but that could be as simple as binary dip-switches that microprocessor monitors.

The dip-switch solution is actually used for concert lighting systems, which also use a digital

control scheme. After a single audio channel is isolated the microprocessor would need to

output that channel to be converted into a PWM-type audio signal.

The easiest way to convert the signal into a PWM-type audio signal would be to have

the embedded system output a PCM signal. In fact, as mentioned earlier, AES50-2005 uses

PCM to encode each individual audio channel, so converting to PCM would be as simple as

tuning in to one specific channel and ignoring the rest. Once a single-channel PCM signal is

created it would need to be converted into a PWM-type signal. There are numerous designs

for PCM to PWM converters, and depending on the exact needs of the system, a design

could be developed from scratch. This type of converter could be designed using a Digital

Signal Processor (DSP) or could be implemented with analog circuitry. DSPs are usually

much easier to troubleshoot as the code contained on the chip can be easily modified, but

DSPs are complicated components and can be relatively expensive. On the other hand,

analog circuits require more design work and are much harder to modify once the circuit is

laid out on a Printed Circuit Board (PCB), but because individual analog components are

extremely inexpensive, an analog circuit may be cheaper to mass produce. Regardless of

whether a DSP or analog circuitry is used, the system could be tailored with various filters

to minimize distortion and noise in the audio signal. An added benefit of using a PCM to

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PWM converter is that an amplifier accessory could be a USB device that outputs a PCM

signal from a personal computer directly to the amplifier. Directly connecting a computer

through a USB port would require additional circuitry and computer software to emulate

a sound card, but it would result in a final product with much greater capabilities than

anything available on the market today.

The development of a Class D audio amplifier with any type of digital interface is in-

evitable because the professional audio market is slowly moving towards a digital standard.

At this point in time, however, there is no single defined digital standard that every manu-

facturer recognizes, which is greatly hampering the movement to an all digital solution. It

appears at this point that the only way a digital audio standard will be adopted is by various

manufacturers beginning to support one standard. The AES50-2005 standard appears to be

adequate for this task, but it has yet to be used in any large capacity. This would require

cooperation between digital mixing console manufacturers, digital snake manufacturers, and

amplifier manufacturers, something that does not appear likely to happen in the near future.

If proof of concept designs are created they may spur movement towards a unifying standard,

which would have an extremely positive effect on the professional audio market.

Below is a table to help summarize some of the more important differences between

analog and digital audio with regard to the live audio market:

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Analog Audio Digital Audio (AES50-2005)

Physical Cabling Specialized ”Snake” CAT5 or Twisted Pair

Large, heavy, expensive

Interface Specialized snake head/tail. RJ-45 connector: Individual

One XLR connector per channel channels controlled by digital interface.

Noise Susceptible to crosstalk and EMI No noise picked up in cable run

Number of channels Each additional channel CAT5-48 channels

requires more copper CAT6-384 channels

Length Up to 500ft (150m) Up to 330ft(100m) per leg

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